cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Pseudo Rotation Curve connecting the Galaxy, Dark Halo, and Local Group
Creators: name: Sofue, Yoshiaki
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We construct a Galacto-Local Group rotation curve, combining the Galactic rotation curve with a diagram, where galacto-centric radial velocities of outer globular clusters and member galaxies of the Local Group are plotted against their galacto-centric distances. The high-velocity ends of this pseudo rotation curve within a radius R ~ 150 kpc are well traced by a rotation curve calculated for the NFW (Navaro, Frenk, White) and Burkert dark halo models. The NFW model indicates that the Galaxy's mass within 385 kpc, half distance to M31, is ~ 4 x 10^{11}M_{sun}. High-velocity ends of the pseudo rotation curve for the entire Local Group up to 1.5 Mpc indicate isothermal nature with a terminal velocity of ~ 200 km/s. In order for the Local Group to be gravitationally bound, an order of magnitude larger mass than those of the Galaxy and M31 is required. This fact indicates that the Local Group contains dark matter of mass ~ 5 x 10^{12}M_{sun} filling the space between the Galaxy and M31. The mass density of the Galactic dark halo becomes equal to that of the Local Group's dark matter at R ~ 100 kpc, beyond which the intracluster dark matter dominates. If we define the Galaxy's radius at this distance, the enclosed Galactic mass is ~ 3 x 10^{11}M_{sun}. We comment on the barionic matter fraction of galaxies in the Local Group.
description: PASJ in press, 10 pages
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÑÑÑÐºÑÑÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð°Ð¿ÑÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ»Ð¾Ñ Ð¿ÑÐ¸ Ñ Ð¾Ð»Ð¾Ð´Ð½Ð¾Ð¼ Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¼ Ð½Ð°Ð¿ÑÐ»ÐµÐ½Ð¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ³Ð¾ÑÐ¸Ð½, Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¼ÐµÑÐ¾Ð´Ñ Ð½Ð°Ð¿ÑÐ»ÐµÐ½Ð¸Ñ Ð¼ÐµÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÑÑÑÐ¸Ð¹
Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð½Ð°Ð¿ÑÐ»ÐµÐ½Ð¸Ðµ
ÑÑÑÑÐºÑÑÑÐ° Ð¿Ð¾ÐºÑÑÑÐ¸Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»Ð¾Ñ Ð¿Ð¾ÐºÑÑÑÐ¸Ñ Ð¿ÑÐ¸ ÑÐ¾Ð»Ð¾Ð´Ð½Ð¾Ð¼ Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¼ Ð½Ð°Ð¿ÑÐ»ÐµÐ½Ð¸Ð¸. ÐÐ¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, Ð´Ð²ÑÑ Ð³Ð»Ð°Ð² Ð¸ Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ñ. ÐÐ¾ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÐµÑÑÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¼Ñ, ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÑÐµÑÑÑ ÑÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, ÑÐºÐ°Ð·ÑÐ²Ð°ÐµÑÑÑ Ð¾Ð±ÑÐµÐºÑ Ð¸ Ð¿ÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐµÑÐ²Ð°Ñ Ð³Ð»Ð°Ð²Ð° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð², Ð² Ð½ÐµÐ¹ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÐºÑÐ°ÑÐºÐ¾ Ð²ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð³Ð°Ð·Ð¾Ð²Ð¾Ð³Ð¾ Ð½Ð°Ð¿ÑÐ»ÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ ÑÐ¾Ð»Ð¾Ð´Ð½Ð¾Ðµ Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð½Ð°Ð¿ÑÐ»ÐµÐ½Ð¸Ðµ. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÐµÑÑÑ ÑÑÐ°Ð¿ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ Ñ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸ÐµÐ¼ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ¾ÑÐ¾Ð³ÑÐ°ÑÐ¸ÑÐ¼Ð¸ ÑÑÑÑÐºÑÑÑÑ Ð¿Ð¾ÐºÑÑÑÐ¸Ñ. ÐÐ°ÐºÐ»ÑÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²ÑÐ²Ð¾Ð´Ñ Ð¿Ð¾ Ð¿ÑÐ¾Ð´ÐµÐ»Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ.
Scaling properties of many-fermion systems from MCRG studies
Creators: name: Hasenfratz, Anna
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Monte Carlo renormalization group methods were designed to study the phase structure and critical behavior of statistical systems. They are well suited to determine the running coupling and to investigate the properties of fixed points of gauge-fermion models, including the existence of conformal infrared fixed points in many-fermion systems. I discuss the implementation of the 2-lattice matching method and present results for SU(3) gauge theories with N_f=0,12 and 16 fundamental fermion flavors.
description: 7 pages, 2 figures. Contribution to the "XXVII International Symposium on Lattice Field Theory", July 26-31, 2009, Peking University, Beijing, China
E se la materia oscura si consumasse?
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2014

È difficile immaginarselo visto che di essa nulla si conosce, ma la materia oscura starebbe consumandosi a favore dell'energia oscura. È quanto afferma uno studio condotto da un gruppo di ricercatori delle Università di Roma “La Sapienza” e Portsmouth, pubblicato su Physical Review Letters
Z_N-Invariant Subgroups of Semi-Simple Lie Groups
Creators: name: Ahsan, M. K.
name: Hubsch, T.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We employ Mathematica to find $Z_N$-invariant subgroups of $E_8$ for application in M-theory. These $Z_N$-invariant subgroups are phenomenologically important and in some cases they resemble the gauge groups of our real world. We present a specific example of $Z_7$-invariant subgroups of $E_8$, which turn up in orbifold compactification of M-theory. Moreover, the procedure can be applied for any $Z_N$ group that acts by shifts (translations) in the root lattice of semisimple Lie groups with $A_n,B_n,C_n,D_n,E_6,E_7$ and $E_8$ factors.
description: Update reflects some corrections and streamlined results hastened by the journal Referee; LaTeX 3 times for correct "longtable" processing
Sibianor kenyaensis Logunov 2001
Creators: name: Logunov, Dmitri
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Salticidae
Sibianor
Sibianor kenyaensis

description: Sibianor kenyaensis Logunov, 2001 Figs 42-44 Identification. Logunov (2001: figs 292, 293). Material examined. BOTSWANA: 1♁ (BMNH), Okavango, Maxwee, Mopane woodland (pitfall traps), 21.11.1975, ARS. Comments. This is the first record of S. kenyaensis following its original description and a new record outside the type locality (Kenya: Kilifi).
description: Published as part of Logunov, Dmitri, 2009, Further notes on the Harmochireae of Africa (Araneae, Salticidae, Pelleninae), pp. 265-290 in ZooKeys 16 (16) on page 285, DOI: 10.3897/zookeys.16.227, http://zenodo.org/record/576485
description: {"references": ["Logunov DV (2001; for 2000) A redefinition of the genera Bianor Peckham & Peckham, 1885 and Harmochirus Simon, 1885, with the establishment of a new genus Sibianor gen. n. (Araneae: Salticidae). Arthropoda Selecta 9 (4): 221 - 286."]}
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÑÐµÐ¼ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ¼Ð¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð´Ð»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ "61 ÐÐ¢Ð Ð")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¸Ð½ÑÐºÐ¸Ð½Ð°, ÐÐ»ÐµÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð±ÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑ
ÑÐ¸ÑÑÐµÐ¼Ñ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ
Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
Ð³ÑÐ°ÑÐ¸Ðº Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ°
Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð²
ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð°

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐ¾Ð¹ ÑÐ²Ð»ÑÐµÑÑÑ Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÑÐµÐ¼ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ¼Ð¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð´Ð»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ "61 ÐÐ¢Ð Ð"). Ð Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð¾Ð±ÑÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÐÐ Â«61 ÐÐ¢Ð ÐÂ», ÑÑÑÑÐºÑÑÑÐ° ÐµÐ³Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° Ð¸ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ.
T-test u stroke studiji i studiji spavanja
Creators: name: Miljković, Nadica
Publisher: name: Zenodo
Year: 2023
Subjects: R programming
Rstats
t-test

description: Jedanaesta vežba za predmet Tehnike obrade biomedicinskih signala na master akademskim studijama na Elektrotehničkom fakultetu Univerziteta u Beogradu.
Dynamics of planets in retrograde mean motion resonance
Creators: name: Gayon, Julie
name: Bois, Eric
name: Scholl, Hans
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: In a previous paper (Gayon & Bois 2008a), we have shown the general efficiency of retrograde resonances for stabilizing compact planetary systems. Such retrograde resonances can be found when two-planets of a three-body planetary system are both in mean motion resonance and revolve in opposite directions. For a particular two-planet system, we have also obtained a new orbital fit involving such a counter-revolving configuration and consistent with the observational data. In the present paper, we analytically investigate the three-body problem in this particular case of retrograde resonances. We therefore define a new set of canonical variables allowing to express correctly the resonance angles and obtain the Hamiltonian of a system harboring planets revolving in opposite directions. The acquiring of an analytical "rail" may notably contribute to a deeper understanding of our numerical investigation and provides the major structures related to the stability properties. A comparison between our analytical and numerical results is also carried out.
description: 15 pages, 3 figures, accepted for publication in Celestial Mechanics and Dynamical Astronomy (January 28, 2009)
Fabiola Gianotti a capo del CERN
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2014

L’Italia ha un rapporto speciale con il CERN,  dal suo inizio, con Edoardo Amaldi tra i padri fondatori, ai successi degli esperimenti LHC, a maggioranza diretti da fisici italiani, suggellati dalla scoperta del bosone di Higgs, passando per il premio Nobel a Carlo Rubbia, anche lui direttore generale, come pure Luciano Maiani. La gioia di Ferroni presidente dell'INFN e i complimenti di Bignami, Presidente INAF
Conferma italiana per la supernova in M61
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2014

Si chiama SN 2014dt ed è una supernova di tipo Iax. A scoprirla, mercoledì scorso, un astrofilo giapponese. Ma a confermarne la natura e a classificarla sono stati, rispettivamente, tre astrofili di Remanzacco e – usando il telescopio di Asiago – un team dell’INAF di Padova
title: ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¿Ð¸ÑÐµÐ»Ð¸Ð°Ð»ÑÐ½ÑÑ ÐºÐ»ÐµÑÐ¾Ðº Ð½Ð°ÑÑÐ¶Ð½Ð¾Ð¹ Ð¾Ð±Ð¾Ð»Ð¾ÑÐºÐ¸ Ð³Ð»Ð°Ð·Ð½Ð¾Ð³Ð¾ ÑÐ±Ð»Ð¾ÐºÐ° Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÐµÑÑ-ÑÐ¸ÑÑÐµÐ¼ Ð¿ÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð»Ð¸Ð¿Ð¾ÑÐ¾Ð¼Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ ÑÑ Ð¸Ð½Ð¾Ñ ÑÐ¾Ð¼Ð°
title: Epithelial cells of the outer shell of the eyeball as test systems in the development of a liposomal form of echinochrome
Creators: name: ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÐµÑ-Ð¡Ð¸Ð½ÐºÐ»ÐµÑ, Ð­.
name: ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ¾Ð²Ð°, Ð¡.
name: ÐÐ°ÑÐ²Ð¸Ñ, Ð.
name: ÐÐ´Ð¾Ð¼ÐµÐ½ÐºÐ¾, Ð.
name: ÐÐ¾ÑÐ±Ð°Ñ, Ð.
name: ÐÑÐ°Ð²ÑÐµÐ½ÐºÐ¾, Ð.
name: ÐÑÐ¼Ð°Ðº, Ð.
name: ÐÐ¸ÑÐ°Ð¹Ð»Ð¾Ð²Ð°, Ð.
name: ÐÐ»Ð¸Ð½Ð¾Ð²Ð°, Ð.
name: "ÐÐ¾Ð»Ð»ÐµÐºÑÐ¸Ð¸ ÐºÑÐ»ÑÑÑÑ ÐºÐ»ÐµÑÐ¾Ðº ÑÐµÐ»Ð¾Ð²ÐµÐºÐ° Ð¸ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÑ : ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð²ÑÐ·Ð¾Ð²Ñ Ð¸ ÑÐµÑÐµÐ²ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ", Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ ÑÐºÐ¾Ð»Ð°-ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2022; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: ÐÐ»ÐµÑÐºÐ° (Ð±Ð¸Ð¾Ð».)
Ð»Ð¸Ð¿Ð¾ÑÐ¾Ð¼Ñ

description: Ð Ð½Ð°ÑÐµÐ¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ CRG/Ech-containing liposomes Ð±ÑÐ»Ð° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð»Ð¸Ð¿Ð¾ÑÐ¾Ð¼, Ð½ÐµÑÑÑÐ¸Ñ ÑÑÐ¸Ð½Ð¾ÑÑÐ¾Ð¼ (Ech) Ð¸ ÐºÐ°ÑÑÐ°Ð³Ð¸Ð½Ð°Ð½ (CRG), Ð¸ Ð¸Ñ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ ÑÑÑÑÐºÑÑÑÐ½ÑÑ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð² Ð½Ð° Ð¶Ð¸Ð·Ð½ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ ÐºÑÐ»ÑÑÐ¸Ð²Ð¸ÑÑÐµÐ¼ÑÑ ÐºÐ»ÐµÑÐ¾Ðº. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÐµÑÑ-ÑÐ¸ÑÑÐµÐ¼ Ð±ÑÐ»Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð»Ð¸Ð½Ð¸Ð¸ ÑÐ¿Ð¸ÑÐµÐ»Ð¸Ð°Ð»ÑÐ½ÑÑ ÐºÐ»ÐµÑÐ¾Ðº Ð½Ð°ÑÑÐ¶Ð½Ð¾Ð¹ Ð¾Ð±Ð¾Ð»Ð¾ÑÐºÐ¸ Ð³Ð»Ð°Ð·Ð½Ð¾Ð³Ð¾ ÑÐ±Ð»Ð¾ÐºÐ°: ÐºÐ»ÐµÑÐºÐ¸ ÐºÐ¾Ð½ÑÑÐ½ÐºÑÐ¸Ð²Ñ (Chang Conjunctiva, Clone 1-5c-4) Ð¸ ÑÐ¿Ð¸ÑÐµÐ»Ð¸Ñ ÑÐ¾Ð³Ð¾Ð²Ð¸ÑÑ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ° (HCE). Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¾ÑÐµÐ½ÐºÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ ÐÐ¢Ð¢-ÑÐµÑÑ Ð¸ Ð¼Ð¾ÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·.
Stochastic Coherence in an Oscillatory Gene Circuit Model
Creators: name: Hilborn, Robert C.
name: Erwin, Jessie D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Molecular Networks (q-bio.MN)
subject: FOS: Biological sciences

description: We show that noise-induced oscillations in a gene circuit model display stochastic coherence, that is, a maximum in the regularity of the oscillations as a function of noise amplitude. The effect is manifest as a system-size effect in a purely stochastic molecular reaction description of the circuit dynamics. We compare the molecular reaction model behavior with that predicted by a rate equation version of the same system. In addition, we show that commonly used reduced models that ignore fast operator reactions do not capture the full stochastic behavior of the gene circuit. Stochastic coherence occurs under conditions that may be physiologically relevant.
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÑÑÐ»ÐºÐ°Â»
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÐºÐ¸ÑÐ¸Ð½Ð°, ÐÑÐµÐ½Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð²ÑÑÐ»ÐºÐ°
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ñ
Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ°

description: Ð Ð¿ÐµÑÐ²Ð¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÑÑÐ»ÐºÐ°Â», Ð²ÑÐ±ÑÐ°Ð½ ÑÐ¿Ð¾ÑÐ¾Ð± Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸, Ð²ÑÐ±ÑÐ°Ð½Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐµÐ¶ÑÑÐ¸Ð¹ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ Ð´Ð»Ñ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÑÐ½ ÑÐ°ÑÑÑÑ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¸ Ð½Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹.
ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐ¾ÐºÐ°ÑÐ½ÑÐ¹ ÑÑÑÑÐºÑÐ»Ð°ÑÐºÐ¾Ð²ÑÐ¹ Ð¿Ð°ÑÑÐ¾Ð½ Ð¸ Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ¸Ð»Ð¾Ð²ÑÐµ ÑÐ°ÑÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¿Ð°ÑÑÐ¾Ð½Ð°.
Ð ÑÑÐµÑÑÐµÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¿Ð¾ÑÑÐ´Ð¾Ðº ÑÐ°ÑÑÑÑÐ° Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸Ð·Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÐ·ÑÐ°.
Mergers and Disk Survival in LCDM
Creators: name: Bullock, James S.
name: Stewart, Kyle R.
name: Purcell, Chris W.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Disk galaxies are common in our universe and this is a source of concern for hierarchical formation models like LCDM. Here we investigate this issue as motivated by raw merger statistics derived for galaxy-size dark matter halos from LCDM simulations. Our analysis shows that a majority (~70%) of galaxy halos with M = 10^12 M_sun at z=0 should have accreted at least one object with mass m > 10^11 M_sun ~ 3 M_disk over the last 10 Gyr. Mergers involving larger objects should have been rare, and this pinpoints m/M = 0.1 mass-ratio mergers as the most worrying ones for the survival of thin galactic disks. Motivated by these results, we use use high-resolution, dissipationless N-body simulations to study the response of stellar Milky-Way type disks to these common mergers and show that thin disks do not survive the bombardment. The remnant galaxies are roughly three times as thick and twice as kinematically hot as the observed thin disk of the Milky Way. Finally, we evaluate the suggestion that disks may be preserved if the mergers involve gas-rich progenitors. Using empirical measures to assign stellar masses and gas masses to dark matter halos as a function of redshift, we show that the vast majority of large mergers experienced by 10^12 M_sun halos should be gas-rich (f_gas > 0.5), suggesting that this is a potentially viable solution to the disk formation conundrum. Moreover, gas-rich mergers should become increasingly rare in more massive halos > 10^12.5 M_sun, and this suggest that merger gas fractions may play an important role in establishing morphological trends with galaxy luminosity.
description: 9 pages, 6 figures; Invited Contribution, IAU Symposium 254, The Galaxy Disk in Cosmological Context
1500 immagini in 5 minuti
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2014

Si tratta della missione RAISE (short for Rapid Acquisition Imaging Spectrograph Experiment), un razzo sonda destinato, nei suoi cinque minuti di missione effettiva, a scattare 1500 immagini del sole, nella frequenza dell'estremo ultravioletto
title: ÐÑÐ¾ÐµÐºÑ Ð¾ÑÐ´ÐµÐ»ÑÐ½Ð¾ ÑÑÐ¾ÑÑÐµÐ¹ Ð²Ð¾Ð´Ð¾Ð³ÑÐµÐ¹Ð½Ð¾Ð¹ Ð³Ð°Ð·Ð¾Ð²Ð¾Ð¹ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´Ð»Ñ Ð°Ð´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð´Ð°Ð½Ð¸Ð¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð§Ð°Ð¿Ð»ÑÐ³Ð¸Ð½, ÐÐ°ÐºÑÐ¸Ð¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐºÐ¾ÑÐµÐ»ÑÐ½ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸
Ð³Ð¾ÑÐµÐ»Ð¾ÑÐ½ÑÐµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°
Ð½Ð°ÑÐ¾Ñ
ÑÐµÐ¿Ð»Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ðµ
Ð²ÐµÐ½ÑÐ¸Ð»ÑÑÐ¸Ñ

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐµÐ¿Ð»Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÐµÐ¹. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐµÐ¿Ð»Ð¾Ð²ÑÐµ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸. ÐÐ¾Ð´Ð¾Ð±ÑÐ°Ð½Ñ ÐºÐ¾ÑÐµÐ»ÑÐ½ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾-Ð²Ð°Ð½Ð¸Ðµ Ð´Ð»Ñ Ð¸Ñ Ð¿Ð¾ÐºÑÑÑÐ¸Ñ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ð° ÑÐµÐ¿Ð»Ð¾Ð²Ð°Ñ ÑÑÐµÐ¼Ð°. ÐÐ·ÑÑÐµÐ½Ñ Ð¸ ÑÑÑÐµÐ½Ñ Ð² Ð¿ÑÐ¾ÐµÐºÑÐµ: Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð¾ÑÑÐ°Ð½Ñ ÑÑÑÐ´Ð°, ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð½Ð¾ÑÐ¼Ñ, Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ ÐºÐ¾ÑÐµÐ»ÑÐ½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº.
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ¾Ð²ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹ Ð½Ð° Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ðµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð² Ñ Ð¾Ð´Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»Ð³Ð¾Ð²Ð°, ÐÐ»Ð¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÑÑÐµÑÑ
ÑÑÑÐµÑÑÐ¾Ð²Ð°Ñ ÑÐ¸ÑÑÐ°ÑÐ¸Ñ
ÑÑÑÐµÑÑÐ¾ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
ÑÑÑÐµÑÑÐ¾Ñ
Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ñ

description: Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: Ð²ÑÑÐ²Ð¸ÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ° Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð² Ð²ÑÐ·Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÑ Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ðµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð½Ð¾Ð²Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼ÐµÑÐ¾Ð´Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¾ÑÑ Ð°Ð½ÐºÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐµÐ´Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð² Ð Ð¾ÑÑÐ¸Ð¸. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÑÑÐµÑÑ, ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ ÑÑÑÐµÑÑÐ°, Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸, Ð² ÐºÐ¾ÑÐ¾ÑÑÑ ÑÑÑÐ´ÐµÐ½Ñ Ð¼Ð¾Ð¶ÐµÑ Ð¿Ð¾Ð´Ð²ÐµÑÐ³Ð°ÑÑÑÑ ÑÑÑÐµÑÑÑ. ÐÑÐ´ÐµÐ»ÑÑÑÑÑ ÑÐ°ÐºÑÐ¾ÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÑÑ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐ¸Ð»ÑÐ½Ð¾Ðµ ÑÑÑÐµÑÑÐ¾Ð²Ð¾Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° ÑÑÑÐ´ÐµÐ½ÑÐ° Ð² ÑÐ¾Ð´Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÐ±Ð»Ð°ÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ: Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¸ Ð²ÑÐ²Ð¾Ð´Ñ, ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸ÐµÑÑ Ð² ÑÐ°Ð±Ð¾ÑÐµ, Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ñ Ð´Ð»Ñ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐµÐ¹ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¼ÐµÑÐ¾Ð´Ð¸Ðº Ð±Ð¾ÑÑÐ±Ñ ÑÐ¾ ÑÑÑÐµÑÑÐ¾Ð¼ Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð¿ÑÐµÐ´Ð¾ÑÐ²ÑÐ°ÑÐµÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ° Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð² Ð²ÑÑÑÐµÐ¼ ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸.
Lo spettacolo del Sole su Titano
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2014

La sonda della NASA Cassini ha catturato i brillanti raggi solari riflessi dalla superficie piatta e liscia dei mari e dei bacini che si trovano al Polo Nord della luna più grande di Titano. Il fenomeno è quello della riflessione speculare
Measurement of Mid-rapidity Inclusive Jet Cross Section in $pp$ Collisions at $\sqrt{s} = 200$ GeV
Creators: name: Kalinkin, Dmitrii
Publisher: name: Zenodo
Year: 2022
Subjects: HEP
QCD
Jets

description: The cross section for inclusive jet production in high-energy 𝑝𝑝 collisions is well described by pQCD in the collinear factorization framework, which, together with its high rate and clear signal, makes it a key observable to study the proton structure. For 𝑝𝑝 collisions at RHIC at a center-of-mass energy of √𝑠 = 200 GeV, the STAR detector provides jet measurements at 0.07 ≲ 𝑥𝑇 ≡ 2𝑝T;jet/√𝑠 ≲ 0.5. At these kinematics, the direct scattering on gluons inside the colliding protons contributes at least half of the total jet production cross section. Measurements of the inclusive jet cross section at RHIC, together with the past Deep Inelastic Scattering measurements, can provide improved constraints on the gluon Parton Distribution Function at high 𝑥.
Una girandola di stelle nel Triangolo
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2014

La splendida galassia a spirale nella costellazione del Triangolo, recentemente ripresa in dettaglio dal telescopio VST dell’ESO, è uno degli oggetti celesti visibili, con l’aiuto di un binocolo, nel cielo serale di novembre. I consigli per osservarla insieme alle costellazioni, ai pianeti e ai principali fenomeni celesti di questo mese
Semiclassical Analysis of Constrained Quantum Systems
Creators: name: Tsobanjan, Artur
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Exact procedures that follow Dirac's constraint quantization of gauge theories are usually technically involved and often difficult to implement in practice. We overview an "effective" scheme for obtaining the leading order semiclassical corrections to the dynamics of constrained quantum systems developed elsewhere. Motivated by the geometrical view of quantum mechanics, our method mimics the classical Dirac-Bergmann algorithm and avoids direct reference to a particular representation of the physical Hilbert space. We illustrate the procedure through the example of a relativistic particle in Minkowski spacetime.
description: 8 pages, Proceedings of "The Planck Scale" (XXV Max Born Symposium, Wroclaw)
Soil texture of Pinus ponderosa plant communities in British Columbia
Creators: name: Ogilvie, Robert Townley
Publisher: name: University of British Columbia
Year: 2012

description: The field, work for this investigation was carried out in the summer of 1952, during this time soil samples and field notes were made. Further soil samples were secured in the summer of 1953, The area in which the yellow pine communities were studied was in the Okanagan, Similkameen, Nicola and South Thompson valleys as well as the southern Cariboo in the vicinity of Clinton, The soil samples were air-dried, weighed and the gravel fraction ( particles greater than 2 mm. in diameter) separated by sieve. The gravel fraction was weighed and the percentage determined for each sample. The mechanical analysis was done by means of the Bouyoueos hydrometer Method, following the removal of organic matter by hydrogen peroxide, and carbonates by treatment with hydrochloric acid. The results of the mechanical analysis were expressed in terms of percentages, by weight, of sand, silt and clay on the basis of the soil sample with the gravel removed. Using the textural classification of the United States Department of Agriculture the results were expressed In terms of sandy loam, loam, etc. for each plant community. The ranges in soil texture for each plant community are: Agropyron association - sandy loam to clay loam with extremes of sand and clay. Stipa subassociation - sandy loam. Artemisia subassociation - clay loam. Purshia association – generally sand, occasionally sandy loam. Aristida subassociation- sand to sandy loam. Rhus association - loamy sand with high percentage of gravel. Arctostaphylos association - sandy loam or loamy sand to sand. Arctostaphylos - Calamagrostis association - sand to sandy Calamagrostis association - sandy clay loam to sandy loam. Symphoricarpos association - sandy loam and sandy clay loam.
La luce eso-zodiacale vista da VLTI
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2014

Si tratta della luce stellare riflessa dalla polvere creata dalla collisione tra asteroidi e dall'evaporazione di comete. Polvere di questo tipo è anche all'origine della luce zodiacale nel Sistema Solare. È la prima volta che si effettua un grande studio sistematico intorno a stelle vicine
Galaxy Zoo: l’Universo era già bambino
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2014

Secondo i teorici non si sarebbero dovute formare prima di 8 miliardi di anni fa. Ma le decine di migliaia di immagini di Hubble, classificate dai volontari di Galaxy Zoo, mostrano galassie che a 3mld di anni dal Big Bang (10mld di anni fa) somigliano in tutto e per tutto all’Universo attuale
3D particle observation/monitoring system for COMPACT
Creators: name: Mohr, Daniel P.
name: Knapek, Christina A.
name: Schütt, Stefan
name: Maier, Daniel
name: Melzer, André
Publisher: name: Zenodo
Year: 2024
Subjects: 3D
particle ovservation
particle monitoring
camera
computer vision
computer stereo vision
stereo vision
triangulation
pinhole camera model
Scheimpflug Principle
dusty plasma
complex plasma
COMPACT
microgravity
International Space Station
ISS
data management
fair principle
low Earth orbit

description: The future complex plasma facility COMPACT  will allow the investigation of large three-dimensional complex plasmas under microgravity conditions aboard the International Space Station (ISS). COMPACT is a project with international scientific contributions, supported by space agencies (DLR, NASA, ESA) and NSF.

The most important diagnostic for all dusty plasma facilities on the ISS (e. g. PK3+, PK4) was/is the observation of the dust particles by cameras. Apart from individual attempts to obtain 3D positions (e. g. doi 10.48550/arXiv.1912.04333), it has not yet been possible to measure this information on the ISS.

For COMPACT for the first time a specially designed 3D particle observation/monitoring system is intended. This system consists of the camera setup (e. g. doi 10.1063/1.3589858), the recording hardware and software as well as the evaluation software (e. g. doi 10.3390/jimaging5020030). The necessary metadata for data management will be recorded already during the data acquisition process.

We present concepts for the camera setup as well as concepts for the evaluation software.

This work is funded by DLR/BMWi (FKZ 50WP0700, 50WM1441, 50WM2161).
Higher order invariants in the case of compact quotients
Creators: name: Deitmar, Anton
Publisher: name: arXiv
Year: 2010
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: We present the theory of higher order invariants and higher order automorphic forms in the simplest case, that of a compact quotient. In this case many things simplify and we are thus able to prove a more precise structure theorem than in the general case.
description: 25 pages, LATeX. arXiv admin note: text overlap with arXiv:0811.1088
COMPACT: Project Status and Research Data Managment
Creators: name: Mohr, Daniel P.
name: Knapek, Christina A.
name: Schütt, Stefan
name: Maier, Daniel
name: Melzer, André
name: Couedel, Lenaic
name: Dove, Adrienne
name: Goree, John
name: Konopka, Uwe
name: Ratynskaia, Svetlana
name: Thoma, Markus H.
name: Thomas, Hubertus M.
name: Wang, Zhehui
name: Zaussinger, Florian
Publisher: name: Zenodo
Year: 2025
Subjects: dusty plasma
complex plasma
COMPACT
microgravity
International Space Station
ISS
low Earth orbit
data management
fair principle

description: Complex, or dusty, plasmas consist of micrometer-sized grains that are injected into a low-temperature noble gas discharge. The grains become charged and interact with each other via a screened Coulomb potential. On ground, gravity compresses the system and prevents the formation of larger, three-dimensional particle clouds.
The future complex plasma facility COMPACT will allow the investigation of large three-dimensional complex plasmas under microgravity conditions aboard the International Space Station (ISS).
COMPACT is a project with international scientific contributions, funded by space agencies (DLR, NASA). The industry phase B is currently underway and will be finished in 2025.
Data generated by experiments on the ISS are of significant importance, as repeating an experiment can be extremely challenging and time-consuming. Therefore, it is crucial to design data management and handling strategies at an early stage to ensure efficient and reliable data processing.
We present the objectives of COMPACT, the project status, and first concepts for the handling of research data acquired with COMPACT following the FAIR principles.
This work is funded by DLR/BMWi (FKZ 50WM2161).
PERFORMING PARENTHOOD: AN ANALYSIS OF MOTHERHOOD AND FATHERHOOD ON TWITTER
Creators: name: Borlase, Kaya
Publisher: name: University of Chicago
Year: 2023
Subjects: subject: parenthood
subject: motherhood
subject: fatherhood
subject: twitter
subject: sentiment analysis
subject: text embedding

description: A growing shift in gender roles in society seems to have infiltrated most areas of life, including family relationships such as parental roles. Existing research shows that both men and women are increasing reporting a desire to have more equality in their parenting roles and tasks. However, during the COVID-19 pandemic, there appeared to be “motherhood penalty” that pushed mothers back into traditional roles. In this thesis, I explore the extent to which parental roles translated online pre- and post- pandemic using a corpus of Tweets posted in 2019 and 2022 that contained the hashtags #DadLife or #MomLife. I examine the differences in tweets posted by fathers and mothers through frequency analysis, sentiment analysis, and text embedding. Results show a reinforcement of the traditional stereotypes about roles that mothers have versus fathers have including both physical and emotional roles; however, there is some overlap between these roles as well. The differences in role performance align with the “motherhood penalty” that occurred during the pandemic and translated directly online. In summary, while gender roles have shifted, the underlying expectations of the parental roles that mothers have and fathers have continue to persist in the digital space of Twitter, especially post-pandemic
Un pianeta poco puntuale
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2014

Le sue anomalie nei tempi di transito davanti alla sua stella madre avevano eluso gli algoritmi automatici che gli astronomi utilizzano per individuare gli esopianeti. Ma non gli occhi dei tanti volontari che partecipano al programma Planet Hunters. E così, dopo ulteriori indagini, ecco scoperto PH3c, un nuovo pianeta extrasolare. Il commento di Valerio Nascimbeni (INAF)
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° ÑÑÑÐ¸ÑÑÑÐºÐ¾Ð¹ Ð¸Ð½Ð´ÑÑÑÑÐ¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¸Ðº
titleType: Subtitle
Creators: name: ÐÑÑÑÑÐ¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
name: ÐÐ¾ÑÐ¾Ð·Ð¾Ð²Ð°, ÐÐ°ÑÐ¸Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2017
Subjects: ÑÑÑÐ¸Ð·Ð¼
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¸Ðº Ð½Ð°ÑÐµÐ»ÐµÐ½ Ð½Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ñ ÑÐ¸ÑÐ°ÑÐµÐ»ÐµÐ¹ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð¾ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ¸ÑÑÑÐºÐ¾Ð¹ Ð¸Ð½Ð´ÑÑÑÑÐ¸Ð¸, ÑÐ°ÑÐºÑÑÐ²Ð°ÐµÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ¸ÑÑÑÐºÐ¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ñ ÐµÐ³Ð¾ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÐµÐ¹ Ð¸ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐ¸Ð¼ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ ÑÑÑÐ¸ÑÑÑÐºÐ¾Ð¹ Ð¸Ð½Ð´ÑÑÑÑÐ¸Ð¸. ÐÑÐ´ÐµÐ»ÑÐ½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ¸Ð·Ð¼Ð° Ð² Ð Ð¤. Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» ÑÑÐµÐ±Ð½Ð¸ÐºÐ° Ð´Ð»Ñ Ð¼Ð°ÐºÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐµÐ³Ð¾ ÑÑÐ²Ð¾ÐµÐ½Ð¸Ñ Ð¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð½Ð° Ð¿ÑÐ°ÐºÑÐ¸ÐºÐµ ÑÑÑÐ¸ÑÑÑÐºÐ¾Ð¹ Ð¾ÑÑÐ°ÑÐ»Ð¸ ÑÐ½Ð°Ð±Ð¶ÐµÐ½ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð¸ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ Ð¿ÑÐ¸Ð¼ÐµÑÐ°Ð¼Ð¸, Ð´Ð°Ð½Ð½ÑÐ¼Ð¸ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°Ð±Ð»ÑÐ´ÐµÐ½Ð¸Ð¹, Ð²ÑÐ´ÐµÑÐ¶ÐºÐ°Ð¼Ð¸ Ð¸ ÑÑÑÐ»ÐºÐ°Ð¼Ð¸ Ð½Ð° Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½ÑÐµ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÑ Ð² ÑÑÐµÑÐµ ÑÑÑÐ¸Ð·Ð¼Ð°. ÐÐ»Ñ Ð½Ð°Ð³Ð»ÑÐ´Ð½Ð¾ÑÑÐ¸ ÑÐ°ÑÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° ÑÑÐµÐ±Ð½Ð¸ÐºÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð² Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð²Ð¸Ð´Ðµ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐ½ÐµÑÐµÐ½Ð° Ð² ÐÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ. Ð¡ÑÑÑÐºÑÑÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ ÑÑÐµÐ±Ð½Ð¸ÐºÐ° Ð²ÑÑÑÑÐ¾ÐµÐ½Ð° Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð¤ÐÐÐ¡ ÐÐÐ 3+ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 43.03.02 Â«Ð¢ÑÑÐ¸Ð·Ð¼Â» (Ð±Ð°ÐºÐ°Ð»Ð°Ð²Ñ), Ð¸ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð° Ð´Ð»Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð´Ð°Ð½Ð½Ð¾Ð¼Ñ Ð¸ ÑÑÐ¾Ð´Ð½ÑÐ¼ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 43.03.03 Â«ÐÐ¾ÑÑÐ¸Ð½Ð¸ÑÐ½Ð¾Ðµ Ð´ÐµÐ»Ð¾Â», 43.03.01 Â«Ð¡ÐµÑÐ²Ð¸ÑÂ». Ð£ÑÐµÐ±Ð½Ð¸Ðº ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ Ð¸Ð½ÑÐµÑÐµÑ Ð´Ð»Ñ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ ÑÑÑÐ¸ÑÑÑÐºÑÑ Ð¸Ð½Ð´ÑÑÑÑÐ¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² ÑÑÑÐ¸ÑÑÑÐºÐ¾Ð³Ð¾ ÑÑÐ½ÐºÐ°.
Ag-Cu alloy surfaces in an oxidizing environment: a first-principles study
Creators: name: Piccinin, Simone
name: Stampfl, Catherine
name: Scheffler, Matthias
Publisher: name: arXiv
Year: 2008
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Recent experiments on model catalysts have shown that Ag-Cu alloys have improved selectivity with respect to pure silver for ethylene epoxidation. In this paper we review our first-principles investigations on the (111) surface of this alloy and present new findings on other low index surfaces. We find that, for every surface orientation, the presence of oxygen leads to copper segregation to the surface. Considering the alloy to be in equilibrium with an oxygen atmosphere and accounting for the effect of temperature and pressure, we compute the surface free energy and study the stability of several surface structures. Investigating the dependence of the surface free energy on the surface composition, we construct the phase diagram of the alloy for every surface orientation. Around the temperature, pressure and composition of interest for practical applications, we find that a limited number of structures can be present, including a thin layer of copper oxide on top of the silver surface and copper-free structures. Different surface orientations show a very similar behavior and in particular a single layer with CuO stoichiometry, significantly distorted when compared to a layer of bulk CuO, has a wide range of stability for all orientations. Our results are consistent with, and help explain, recent experimental measurements.
An Axiomatic Setup for Algorithmic Homological Algebra and an Alternative Approach to Localization
Creators: name: Barakat, Mohamed
name: Lange-Hegermann, Markus
Publisher: name: arXiv
Year: 2010
Subjects: subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: 18E10, 18E25, 18G05, 18G10, 18G15, 13H99, 13P10, 13P20

description: In this paper we develop an axiomatic setup for algorithmic homological algebra of Abelian categories. This is done by exhibiting all existential quantifiers entering the definition of an Abelian category, which for the sake of computability need to be turned into constructive ones. We do this explicitly for the often-studied example Abelian category of finitely presented modules over a so-called computable ring $R$, i.e., a ring with an explicit algorithm to solve one-sided (in)homogeneous linear systems over $R$. For a finitely generated maximal ideal $\mathfrak{m}$ in a commutative ring $R$ we show how solving (in)homogeneous linear systems over $R_{\mathfrak{m}}$ can be reduced to solving associated systems over $R$. Hence, the computability of $R$ implies that of $R_{\mathfrak{m}}$. As a corollary we obtain the computability of the category of finitely presented $R_{\mathfrak{m}}$-modules as an Abelian category, without the need of a Mora-like algorithm. The reduction also yields, as a by-product, a complexity estimation for the ideal membership problem over local polynomial rings. Finally, in the case of localized polynomial rings we demonstrate the computational advantage of our homologically motivated alternative approach in comparison to an existing implementation of Mora's algorithm.
description: Fixed a typo in the proof of Lemma 4.3 spotted by Sebastian Posur
title: ÐÑÑÑ Ð»ÐµÐºÑÐ¸Ð¹ Ð¿Ð¾ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð¾Ð¹ Ð¼ÐµÑ Ð°Ð½Ð¸ÐºÐµ. Ð§. 1, Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼ÐµÑ Ð°Ð½Ð¸ÐºÐ° Ð¸ ÑÐ¾Ð¿ÑÐ¾ÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡ÐµÐ¼Ð¸Ð»ÐµÑÐµÐ½ÐºÐ¾, ÐÐ¾ÑÐ¸Ñ
name: ÐÐ¾Ð»ÐµÑÑÐº, ÐÐ»ÐµÐ³
Publisher: name: Ð¡ÐÐ±Ð¢Ð­Ð
Year: 2007
Subjects: ÐÐµÑ Ð°Ð½Ð¸ÐºÐ° Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ
Ð¡Ð¾Ð¿ÑÐ¾ÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ. Ð§Ð°ÑÑÑ 1 (ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ° Ð¸ ÑÐ¾Ð¿ÑÐ¾ÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²) Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ ÐºÐ¾Ð½ÑÐ¿ÐµÐºÑ Ð»ÐµÐºÑÐ¸Ð¹, ÐºÐ¾ÑÐ¾ÑÑÐ¹ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¿Ð¾ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð¾Ð¹ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐµ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐµÑ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Â«Ð¢Ð¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÑÐ¾Ð²Ð°ÑÐ¾Ð²Â».
$B \to K^{\ast}_0(1430) l^{+} l^{-}$ decays in supersymmetric theories
Creators: name: Aslam, M. Jamil
name: Lu, Cai-Dian
name: Wang, Yu-Ming
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The weak decays of $B \to K^{\ast}_0(1430) l^{+} l^{-}$ ($l=μ, τ$) are investigated in Minimal Supersymmetric Standard Model (MSSM) and also in Supersymmetric (SUSY) SO(10) Grand Unified Models. Neutral Higgs bosons are the point of main focus in MSSM because they make quite a large contribution in exclusive $B \to X_{s} l^{+} l^{-}$ decays at large $\tanβ$ regions of parameter space of SUSY models, as part of SUSY contributions is proportional to $\tan^{3}β$. The analysis of decay rate, forward-backward asymmetries and lepton polarization asymmetries in $B \to K^{\ast}_0(1430) l^{+} l^{-}$ show that the values of these physical observables are greatly modified by the effects of neutral Higgs bosons. In SUSY SO(10) GUT model, the new physics contribution comes from the operators which are induced by the neutral Higgs boson penguins and also from the operators with chirality opposite to that of the corresponding Standard Model (SM) operators. SUSY SO(10) effects show up only in the decay $B \to K^{\ast}_0 μ^{+} μ^{-}$ where the transverse lepton polarization asymmetries deviate significantly from the SM value while the effects in the decay rate, forward-backward asymmetries, the longitudinal and normal lepton polarization asymmetries are very mild. The transverse lepton polarization asymmetry is almost zero in SM and in MSSM model, whereas it can reach to -0.3 in SUSY SO(10) GUT model which could be seen at the future colliders; hence this asymmetry observable can be used to discriminate between different SUSY models.
description: 16 pages, 5 figures
title: ÐÐµÑÐ¾Ð´Ñ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸ Ð²ÑÑÑÐµÐ³Ð¾ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ ÑÐµÑÑÑÑÐ½ÑÑ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 5.2.6. ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
titleType: Subtitle
Creators: name: Ð ÑÑÑÐ¸Ðº, ÐÐ°ÑÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2023
Subjects: ÐºÐ°Ð´ÑÐ¾Ð²ÑÐ¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸
ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð°Ð¶Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð´Ð»Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÑÐºÐ¾-Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð° Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ ÑÐµÑÑÑÑÐ½ÑÑ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹ Ð²ÑÑÑÐµÐ³Ð¾ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð²Ð½ÑÑÑÐ¸ ÑÑÑÐ°Ð½Ñ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð½ÐµÑÐ²Ð°ÑÐºÐ¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð².
La Terra è nata bagnata
Creators: Leonardo De Cosmo
Publisher: name: Media Inaf
Year: 2014

La Terra è nata bagnata. A ipotizzarlo è uno studio coordinato da Adam Sarafian dell'Istituto Oceanografico Woods Hole, negli Usa, e pubblicato su Science. L'opinione di Maria Cristina De Sanctis, dell'Istituto di Astrofisica e Planetologia Spaziale dell'INAF
A che ora parte l’asteroide per Marte?
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2014

Sul numero odierno della rivista Nature è comparso un lungo articolo firmato da Richard Binzel, professore di scienze planetarie del MIT, riguardo alla missione NASA Asteroid Redirect Mission, missione che vorrebbe “catturare” un asteroide e usarlo come passaggio verso Marte. Secondo Binzel il programma sarebbe troppo dispendioso e non porterebbe a risultati significativi tali da facilitare il prossimo passo dell’uomo nello spazio: quello verso Marte
title: Ð­ÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÑÑÐ´Ð° ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð¿ÑÑÐ¸ ÐµÐµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÑÐ°Ð¹Ð»Ð¾Ð²Ð°, Ð®Ð»Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÑÑÐ´Ð°
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÑÑÐ´Ð°
Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»
ÑÑÑÐ´Ð¾Ð²ÑÐµ ÑÐµÑÑÑÑÑ
Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÐ¹ ÐÐÐ Â«ÐÐ¸ÑÑÐ°Ð½ ÐÑÐ½ÑÑÑÐºÑÑÑÐ¸Ð½Ð³ Ð ÑÑÂ».
Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ´Ð° ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð¿Ð¾Ð¸ÑÐº Ð¿ÑÑÐµÐ¹ Ð¿Ð¾ ÐµÐµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ.
ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð±Ð°Ð»Ð°Ð½ÑÐ° ÑÐ°Ð±Ð¾ÑÐµÐ³Ð¾ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐ´Ð° Ð±ÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ´Ð° Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
ÐÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐ´ÐµÐ»Ð°Ð½ Ð²ÑÐ²Ð¾Ð´ Ð¾ ÑÐ¾Ð¼, ÑÑÐ¾ ÑÑÐ¾Ð¸Ñ ÑÐ¾ÐºÑÐ°ÑÐ°ÑÑ Ð½Ð¸Ð·ÐºÐ¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð², Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¸ Ð¿Ð¾Ð²ÑÑÐ°ÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ ÑÑÐµÐ´Ð¸ ÑÐ°Ð±Ð¾ÑÐ¸Ñ.
Ð¡Ð´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¹ Ð¾Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ´Ð°.
title: “They Will Live without Law or Religion”: Cádiz, Indigenous People, and Political Change in the Viceroyalty of Peru, 1812–1820
Creators: name: Escanilla Huerta, Silvia
Publisher: name: Duke University Press
Year: 2021

description: This article argues that the impact of the Constitution of Cádiz among Indigenous communities in the Viceroyalty of Peru was significant. In the context of the imperial crisis of the Spanish crown, Indigenous people took the tools that the constitution granted them to increase their level of self-government. Moreover, the changes implemented by the constitution persisted after its abolition, allowing Indigenous people to retain a level of self-government otherwise impossible to conceive after Ferdinand VII restored absolutist rule. In other words, Indigenous communities held on to their jurisdictional authority and refused to surrender the political tools that the constitution had granted them. Their actions demonstrate that the constitution was a watershed moment in the history of the viceroyalty because it inaugurated an era of political change with consequences nobody could predict at the time.
title: Vittefleur_Arbre53
Creators: name: Galinand, Cyrille
name: Université Paris1 Panthéon-Sorbonne
Publisher: name: Archeovision
Year: 2024
Subjects: subject: arborglyphe

description: arborglyphe
description: 1 fichier 3D (ply), 28 fichiers image (jpg)
Il tesoro di CoRoT: una cefeide unica
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2014

Scoperta 'postuma' per il satellite CoRoT, spento lo scorso 17 giugno a seguito di un'avaria. Nel tesoro di dati che ci ha lasciato c'è una variabile Cefeide che pulsa in un modo completamente differente da tutte le altre osservate nella nostra Galassia. Fra gli autori dell'articolo pubblicato su APJ anche Ennio Poretti dell'INAF-Osservatorio Astronomico di Brera