cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Origin of Exponential Star-forming Disks
Creators: name: Wang, Enci
name: Lilly, Simon J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The disk components of galaxies generally show an exponential profile extending over several scale lengths, both in mass and star-formation rate, but the physical origin is not well understood. We explore a physical model in which the galactic gas disk is viewed as a "modified accretion disk" in which coplanar gas inflow, driven by viscous stresses in the disk, provides the fuel for star formation, which progressively removes gas as it flows inwards. We show that magnetic stresses from magneto-rotational instability are the most plausible source of the required viscosity, and construct a simple physical model to explore this. A key feature is to link the magnetic field strength to the local star-formation surface density, $B_{\rm tot} \propto Σ_{\rm SFR}^α$. This provides a feed-back loop between star-formation and the flow of gas. We find that the model naturally produces stable steady-state exponential disks, as long as $α\sim$ 0.15, the value indicated from spatially-resolved observations of nearby galaxies. The disk scale-length $h_{\rm R}$ is set by the rate at which the disk is fed, by the normalization of the $B_{\rm tot}-Σ_{\rm SFR}$ relation and by the circular velocity of the halo. The angular momentum distribution of the gas and stars within the disk is a consequence of the transfer of angular momentum that is inherent to the operation of an accretion disk, rather than the initial angular momentum of the inflowing material. We suggest that magnetic stresses likely play a major role in establishing the stable exponential form of galactic disks.
description: 28 pages, 17 figures. Accepted for publication in ApJ
Additional file 2 of Research hotspots and trends of bone defects based on Web of Science: a bibliometric analysis
Creators: name: Lin, Haixiong
name: Wang, Xiaotong
name: Huang, Minling
name: Li, Zige
name: Shen, Zhen
name: Feng, Junjie
name: Chen, Huamei
name: Wu, Jingjing
name: Gao, Junyan
name: Wen, Zheng
name: Huang, Feng
name: Jiang, Ziwei
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Cancer
subject: Science Policy

description: Additional file 2. Supplementary Table 2 Top 5 jornals in terms of co-cited frequency or centrality
Stress-Testing Cosmic Ray Physics: The Impact of Cosmic Rays on the Surviving Disk of Ram Pressure Stripped Galaxies
Creators: name: Farber, Ryan Jeffrey
name: Ruszkowski, Mateusz
name: Tonnesen, Stephanie
name: Holguin, Paco
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Cluster spiral galaxies suffer catastrophic losses of the cool, neutral gas component of their interstellar medium due to ram pressure stripping, contributing to the observed quenching of star formation in the disk compared to galaxies in lower density environments. However, the short term effects of ram pressure on the star formation rate and AGN activity of galaxies undergoing stripping remain unclear. Numerical studies have recently demonstrated cosmic rays can dramatically influence galaxy evolution for isolated galaxies, yet their influence on ram pressure stripping remains poorly constrained. We perform the first cosmic-ray magneto-hydrodynamic simulations of an $L_{*}$ galaxy undergoing ram pressure stripping, including radiative cooling, self-gravity of the gas, star formation, and stellar feedback. We find the microscopic transport of cosmic rays plays a key role in modulating the star formation enhancement experienced by spirals at the outskirts of clusters compared to isolated spirals. Moreover, we find that galaxies undergoing ram pressure stripping exhibit enhanced gas accretion onto their centers, which may explain the prevalence of AGN in these objects. In agreement with observations, we find cosmic rays significantly boost the global radio emission of cluster spirals. Although the gas removal rate is relatively insensitive to cosmic ray physics, we find that cosmic rays significantly modify the phase distribution of the remaining gas disk. These results suggest observations of galaxies undergoing ram pressure stripping may place novel constraints on cosmic-ray calorimetry and transport.
description: 15 pages, 10 figures, submitted to MNRAS
Catomentosaponin, a new triterpene saponin from the roots of Catunaregam tomentosa
Creators: name: Sutin Kaennakam
name: Kitiya Rassamee
name: Pongpun Siripong
name: Tip-Pyang, Santi
Publisher: name: Taylor & Francis
Year: 2017
Subjects: subject: Biochemistry
subject: Pharmacology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Inorganic Chemistry
subject: Plant Biology

description: A new triterpene saponin, catomentosaponin (1) and 11 known analogues (2–12) were isolated from the roots of Catunaregam tomentosa. The structures of 1–12 were determined on the basis of extensive NMR and MS data analysis. The sugar residues were identified by co-TLC and HPLC analysis after hydrolysis. All isolated compounds were evaluated for their cytotoxicity against KB and HeLa cell lines. Compound 2 showed moderate cytotoxicity against KB cell with IC50 value of 24.84 μM.
The recent LMC-SMC collision: Timing and impact parameter constraints from comparison of Gaia LMC disk kinematics and N-body simulations
Creators: name: Choi, Yumi
name: Olsen, Knut A. G.
name: Besla, Gurtina
name: van der Marel, Roeland P.
name: Zivick, Paul
name: Kallivayalil, Nitya
name: Nidever, David L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present analysis of the proper-motion (PM) field of the red clump stars in the Large Magellanic Cloud (LMC) disk using the Gaia Early Data Release 3 catalog. Using a kinematic model based on old stars with 3D velocity measurements, we construct the residual PM field by subtracting the center-of-mass motion and internal rotation motion components. The residual PM field reveals asymmetric patterns, including larger residual PMs in the southern disk. Comparisons between the observed residual PM field with those of five numerical simulations of an LMC analog that is subject to the tidal fields of the Milky Way and the Small Magellanic Cloud (SMC) show that the present-day LMC is not in dynamical equilibrium. We find that both the observed level of disk heating (PM residual root-mean-square of 0.057$\pm$0.002 mas yr$^{-1}$) and kinematic asymmetry are not reproduced by Milky Way tides or if the SMC impact parameter is larger than the size of the LMC disk. This measured level of disk heating provides a novel and important method to validate numerical simulations of the LMC-SMC interaction history. Our results alone put constraints on an impact parameter $\lesssim$10 kpc and impact timing $
description: 17 pages, 10 figures, resubmitted to AAS Journal
BOSHLANG'ICH SINF O'QUVCHILARIDA DINIY BAG'RIKENGLIK TUSHUNCHALARINI SHAKLLANTIRISH PEDAGOGIK MUAMMO SIFATIDA
Creators: name: Xisomiddinova, Maftuna
Publisher: name: Zenodo
Year: 2024

description: Boshlang‘ich sinf o‘quvchilarini diniy bag‘rikenglik ruhida tarbiyalashimiz o‘zga din vakillariga ehtirom ko‘rsatib, ularga so‘zda va amalda yaxshilik qilish kabi umuminsoniy qadriyatlarni shakllantirish haqida fikr yuritilgan
Comparison between core-collapse supernova nucleosynthesis and meteoric stardust grains: investigating magnesium, aluminium, and chromium
Creators: name: Hartogh, Jacqueline den
name: Petö, Maria K.
name: Lawson, Thomas
name: Sieverding, Andre
name: Brinkman, Hannah
name: Pignatari, Marco
name: Lugaro, Maria
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Isotope variations of nucleosynthetic origin among Solar System's solid samples are well documented, yet the origin of these variations is still uncertain. The observed variability of \iso{54}Cr among materials formed in different regions of the proto-planetary disk has been attributed to variable amounts of presolar chromium-rich oxide (chromite) grains, which exist within the meteoritic stardust inventory and most likely originated from some type of supernova explosions. To investigate if core-collapse supernovae (CCSNe) could be the site of origin of these grains, we analyse yields of CCSN models of stars with initial mass 15, 20 and 25 M$_{\odot}$, and solar metallicity. We present an extensive abundance data set of the Cr, Mg, and Al isotopes as a function of enclosed mass. We find cases in which the explosive C-ashes produce a composition in good agreement with the observed \iso{54}Cr/\iso{52}Cr and \iso{53}Cr/\iso{52}Cr ratios as well as the \iso{50}Cr/\iso{52}Cr ratios. Taking into account that the signal at atomic mass 50 could also originate from \iso{50}Ti, the ashes of explosive He-burning also match the observed ratios. Addition of material from the He ashes (enriched in Al and Cr relative to Mg to simulate the make-up of chromite grains) to the Solar System composition may reproduce the observed correlation between Mg and Cr anomalies, while material from the C-ashes does not present significant Mg anomalies together with Cr isotopic variations. In all cases, non-radiogenic, stable Mg isotope variations dominate over the variations expected from \iso{26}Al.
description: Accepted for publication in ApJ Data available at https://doi.org/10.5281/zenodo.5822654
Is magnetically dominated outflow required to explain GRBs?
Creators: name: Vereshchagin, Gregory
name: Li, Liang
name: Bégué, Damien
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The composition of relativistic outflows producing gamma-ray bursts is a long standing open question. One of the main arguments in favor of magnetically dominated outflows is the absence of photospheric component in their broadband time resolved spectra, with such notable example as GRB 080916C. Here, we perform a time-resolved analysis of this burst and confirm the previous detection of an additional spectral component. We show that this subdominant component is consistent with the photosphere of ultrarelativistic baryonic outflow, deep in the coasting regime. We argue that, contrary to previous statements, the magnetic dominance of the outflow is not required for the interpretation of this GRB. Moreover, simultaneous detection of high energy emission in its prompt phase requires departure from a one-zone emission model.
Pew Research Center: Israel's Religiously Divided Society May 2015 Survey
Creators: name: Neubauer Family Foundation
name: Trusts, The Pew Charitable
Publisher: name: Roper Center for Public Opinion Research
Year: 2020

description: Most important long-term problem (1); personal economic situation (2); important goals in life (6); discrimination against Muslims/homosexuals/secular Jews (Hiloni)/religious Jews (Haredim/Datiim/Masorti)/women/Ethiopian Jews/Mizrahim (7); peace settlement with Palestinians (2); Israel as both halakhah/democratic state (1); halakhah vs. democratic principles in Israel (1); science vs. religion (1); evolution (1); divorce (2); US support of Israel (1); American Jews (3); Jewish settlements helping/hurting Israel (1); possible coexistence of independent Israeli and Palestinian states (1); le'om (nationhood/ethnic affiliation) (1); religious self-identification (3); Jewish (non-religious) self-identification (1); being Jewish/Muslim/Christian/Druze as a matter of religion/ancestry/culture (2); essential parts of being Jewish/Muslim/Christian (25); Jewish/Muslim/Christian/Druze sense of pride/belonging/social responsibility (3); Jewish vs. Israeli primary self-identification (1); long-term survival of Jews (2); antisemitism (2); Jews living anywhere vs. only in Israel (1); Jewish/Muslim/Christian/Druze homogenous close friends (1); Haredi/Dati/Masorti/Hiloni close friends (1); aliyah (immigration of Jews to Israel) (1); do Jews deserve preferential treatment in Israel (1); should Arabs be expelled/transferred from Israel (1); Haredi/Dati/Masorti/Hiloni self-identification (2); child marrying Haredi/Dati/Masorti/Hiloni (4); child marrying Christian/Jew/Muslim (3); activities on Shabbat (3); women praying at the Kotel (Western Wall) (1); Haredi male conscription (1); public transportation used by Haredim (1); Conservative and Reform rabbis (1); religion in government (1); halakhah/Sharia/Bible as law of Israel (1); experiences of Muslims/Christians/Druze (5); Orthodox/Conservative/Reform self-identification (1); observing religious tradition (1); religious service attendance (1); importance of religion (1); importance of being Jewish/Muslim/Christian/Druze (1); belief in higher power (3); Israel God-given to Jews or not (1); beliefs about Jesus (2); Shabbat candles (1); Hanukkah candles (1); pilgrimage to Mecca (1); giving zakat (1); fasting during Ramadan (1); anointing (1); tithing (1); fasting during Lent (1); icons of saints/holy figures (1); keeping kosher (2); eating pork (1); Pesach (Passover) seder (2); fasting during Yom Kippur (1); baptism (1); going to confession (1); studying Torah/Gemara/etc (1); prayer (2); beliefs about Bible (2); one/multiple ways to interpret one's religion (1); one/multiple ways to heaven (1); head coverings (2); Jewish parents (2); ethnic self-identification (1); country of parents' birth (2); active military duty (1); Zionist self-identification (1); place of birth (2); household appliances/modes of transportation (27); respondent beard (1); travel to US (2).
Production Efficiencies of Sound Waves in the Intracluster Medium Driven by AGN Jets
Creators: name: Wang, Shiang-Chih
name: Yang, H. -Y. Karen
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Feedback from active galactic nuclei (AGN) is believed to be the most promising solution to the cooling flow problem in cool-core clusters, though how exactly the jet energy is transformed into heat is a subject of debate. Dissipation of sound waves is considered as one of the possible heating mechanisms; however, its relative contribution to heating remains unclear. To estimate the energy budget for heating, we perform 3D hydrodynamic simulations of AGN jet injections in a Perseus-like cluster and quantify the amount of energy stored in the forms of weak shocks and waves. We find that, for a single jet injection with typical parameters in cool-core clusters, $\sim9\%$ of the total jet energy is stored in compressional waves (including both shocks and waves). However, due to the destructive effects among randomly phased waves as well as the dissipation of shock energies, in our simulations including self-regulated AGN feedback, no more than $3\%$ of the total injected energy goes into compressional waves. We further separate the energy contribution from shocks and waves and find that, for a single outburst, the shocks can only contribute to $\sim20-30\%$ of the total compressional energy in the inner radii, and they dissipate very quickly as they travel outward. However, because of the repeated generation of shocks by multiple AGN outbursts, in the self-regulated case shocks completely dominate over sound waves in the inner region and can still provide $\sim40-50\%$ of the total compressional energy even at outer radii. Our results suggest that the production of sound waves is not as efficient as what was found in previous single-outburst simulations, and thus sound wave dissipation may be a subdominant source of heating in cool-core clusters.
description: 10 pages, 8 figures, accepted to MNRAS
Two cSNPs sites in the fatty acid-binding protein 4 (FABP4) gene and their association analysis with body measurement data in five Chinese cattle breeds
Creators: name: Xu, Jiawei
name: Liu, Xian
name: Cai, Cuicui
name: Su, Woyu
name: Xie, Jianliang
name: Zhang, Zijing
name: Yang, Peng
name: Lyu, Shijie
name: Li, Zhiming
name: Lei, Chuzhao
name: Chen, Hong
name: Wang, Eryao
name: Ru, Baorui
name: Huang, Yongzhen
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified

description: Single nucleotide polymorphisms (SNPs) include the transition and transversion of a single base. In this study, we found two cSNPs (rs110757796 and rs110652478) in the FABP4 (fatty acid-binding protein 4) gene and tested their population genetic parameters in five Chinese cattle breeds. FABP4 is a key marker molecule for lipid production. It plays a crucial role in the growth and development of animals. Thus, we also analyze the association between the two cSNPs of FABP4 gene and body measurement data of Chinese cattle. Our results were indicated that rs110757796 was significantly associated with the chest width in Chinese cattle groups (p < 0.05). In addition, we tested the spatiotemporal expression profile of the bovine FABP4 gene and effect of genetic variation on its expression. It was found that bovine FABP4 gene has tissue-differential expression. Then, the genetic variation located on the exon has a certain effect on the expression of FABP4 gene in bovine muscle. Overall, our results provide that FABP4 could as a candidate gene to improve the progress of cattle molecular breeding.
Pretreatment with N-acetyl cysteine suppresses chronic reactive astrogliosis following maternal nanoparticle exposure during gestational period
Creators: name: Atsuto Onoda
name: Takeda, Ken
name: Umezawa, Masakazu
Publisher: name: Taylor & Francis
Year: 2017
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Pharmacology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 20199 Astronomical and Space Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Early pregnant employees are potentially and unintendedly exposed to industrial chemicals including nanoparticles. Developmental toxicity of nanoparticle exposure has been concerned because exposure to fine particle including carbon black nanoparticle (CB-NP) during the brain developmental stage enhances the risk of brain disorders. Maternal CB-NP exposure dose-dependently induces astrogliosis, which is an abnormal increase in the reactive astrocytes with glial fibrillary acidic protein (GFAP) and aquaporin-4 overexpression due to the destruction of nearby neurons and blood vessels. The present study aimed to investigate protective effects of antioxidants on the histopathological denaturation with astrogliosis following maternal CB-NP exposure in offspring mice, thereby to evaluate the role of oxidative stress on the developmental toxicity. Pregnant ICR mice were treated with CB-NP by intranasal instillation on gestational days 5 and 9. N-acetyl cysteine (NAC) or ascorbic acid was intraperitoneally administered to the pregnant mice 1 h prior to CB-NP instillation. The brains were collected from 6- to 12-week-old offspring mice and analyzed using western blotting and immunohistochemistry. NAC suppressed GFAP overexpression in 6- and 12-week-old offspring mice following maternal CB-NP exposure. However, NAC did not suppress aquaporin-4 overexpression following maternal CB-NP exposure. Ascorbic acid did not suppress, but rather slightly and significantly enhanced the expression of GFAP and aquaporin-4. These results indicate that astrogliosis by maternal CB-NP exposure is partially prevented by NAC pretreatment. Oxidative stress is a possible key factor of developmental neurotoxicity of maternal NP exposure. This study will contribute to elucidating the mechanisms underlying the effects of developmental neurotoxicity of NPs.
Commentary on the clinical and preclinical dosage limits of interstitially administered magnetic fluids for therapeutic hyperthermia based on current practice and efficacy models
Creators: name: Southern, Paul
name: Pankhurst, Quentin A.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer

description: We offer a critique of what constitutes a suitable dosage limit, in both clinical and preclinical studies, for interstitially administered magnetic nanoparticles in order to enable therapeutic hyperthermia under the action of an externally applied alternating magnetic field. We approach this first from the perspective of the currently approved clinical dosages of magnetic nanoparticles in the fields of MRI contrast enhancement, sentinel node detection, iron replacement therapy and magnetic thermoablation. We compare this to a simple analytical model of the achievable hyperthermia temperature rise in both humans and animals based on the interstitially administered dose, the heating and dispersion characteristics of the injected fluid, and the strength and frequency of the applied magnetic field. We show that under appropriately chosen conditions a therapeutic temperature rise is achievable in clinically relevant situations. We also show that in such cases it may paradoxically be harder to achieve the same therapeutic temperature rise in a preclinical model. We comment on the implications for the evidence-based translation of hyperthermia based interventions from the laboratory to the clinic.
MADANIY TADBIRLARDA REPERTUAR TANLASH HUSUSIYATLARI
Creators: name: Nasirdinov, Murot
Publisher: name: Zenodo
Year: 2024

description: Mazkur maqolada mamlakatimizdagi madaniyat sohasidagi islohotlar, madaniy tadbirlarni tashkil etish, so’z ustida ishlash va uning bosqichlari, ijrochilik faoliyati, repertuar tanlash, yakka ijro etiladigan asarlar tahlili haqida batafsil ma’lumot berilgan.
Very Local Interstellar Medium Revealed by Complete Solar Cycle of Interstellar Neutral Helium Observations with IBEX
Creators: name: Swaczyna, P.
name: Kubiak, M. A.
name: Bzowski, M.
name: Bower, J.
name: Fuselier, S. A.
name: Galli, A.
name: Heirtzler, D.
name: McComas, D. J.
name: Möbius, E.
name: Rahmanifard, F.
name: Schwadron, N. A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Space Physics (physics.space-ph)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The IBEX-Lo instrument on board the Interstellar Boundary Explorer (IBEX) mission samples interstellar neutral (ISN) helium atoms penetrating the heliosphere from the very local interstellar medium (VLISM). In this study, we analyze the IBEX-Lo ISN helium observations covering a complete solar cycle, from 2009 through 2020 using a comprehensive uncertainty analysis including statistical and systematic sources.W e employ the Warsaw Test Particle Model to simulate ISN helium fluxes at IBEX, which are subsequently compared with the observed count rate in the three lowest energy steps of IBEX-Lo. The $χ^2$ analysis shows that the ISN helium flows from ecliptic $(λ,β)=(255.59^{\circ}\pm0.23^{\circ}, 5.14^{\circ}\pm0.08^{\circ})$, with speed $v_\text{HP}=25.86\pm0.21$ km s$^{-1}$ and temperature $T_\text{HP}=7450\pm140$ K at the heliopause. Accounting for gravitational attraction and elastic collisions, the ISN helium speed and temperature in the pristine VLISM far from the heliopause are $v_\text{VLISM}=25.9$ km s$^{-1}$ and $T_\text{VLISM}=6150$ K, respectively. The time evolution of the ISN helium fluxes at 1 au over 12 years suggests significant changes in the IBEX-Lo detection efficiency, higher ionization rates of ISN helium atoms in the heliosphere than assumed in the model, or an additional unaccounted signal source in the analyzed observations. Nevertheless, we do not find any indication of the evolution of the derived parameters of ISN helium over the period analyzed. Finally, we argue that the continued operation of IBEX-Lo to overlap with the Interstellar Mapping and Acceleration Probe (IMAP) will be pivotal in tracking possible physical changes in the VLISM.
description: 31 pages, 6 figures, 8 tables, accepted for publication in ApJS
The Magnetic Field versus Density relation in Star-Forming Molecular Clouds
Creators: name: Auddy, Sayantan
name: Basu, Shantanu
name: Kudoh, Takahiro
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We study the magnetic field to density ($B-ρ$) relation in turbulent molecular clouds with dynamically important magnetic fields using nonideal three-dimensional magnetohydrodynamic simulations. Our simulations show that there is a distinguishable break density $ρ_{\rm T}$ between the relatively flat low density regime and a power-law regime at higher densities. We present an analytic theory for $ρ_{\rm T}$ based on the interplay of the magnetic field, turbulence, and gravity. The break density $ρ_{\rm T}$ scales with the strength of the initial Alfvén Mach number $\mathcal{M}_{\rm A0}$ for sub-Alfvénic ( $\mathcal{M}_{\rm A0}<1$) and trans-Alfvénic ($\mathcal{M}_{\rm A0} \sim 1$) clouds. We fit the variation of $ρ_{\rm T}$ for model clouds as a function of $\mathcal{M}_{\rm A0}$, set by different values of initial sonic Mach number $\mathcal{M_{\rm 0}}$ and the initial ratio of gas pressure to magnetic pressure $β_{\rm 0}$. This implies that $ρ_{\rm T}$, which denotes the transition in mass-to-flux ratio from the subcritical to supercritical regime, is set by the initial turbulent compression of the molecular cloud.
description: 6 pages, 3 Figures, 1 online animation, accepted in ApJL
Neutrino Mass from Affleck-Dine Leptogenesis and WIMP Dark Matter
Creators: name: Mohapatra, Rabindra N.
name: Okada, Nobuchika
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Affleck-Dine (AD) mechanism for leptogenesis involves the cosmological evolution of a complex scalar field (AD field) that carries non-zero lepton number. We show how explicit lepton number breaking terms, which involve the AD field needed to implement this scenario combined with fermionic WIMP dark matter, can generate neutrino mass at the one loop level, thus providing a unified framework for solving four major puzzles of the standard model i.e. inflation, baryogenesis, dark matter and neutrino mass. We discuss some phenomenological implications of this model.
description: 14 pages and 2 figures; references updated and some more comments added
Additional file 1 of TRIM18 is a critical regulator of viral myocarditis and organ inflammation
Creators: name: Fang, Mingli
name: Zhang, Ao
name: Du, Yong
name: Lu, Wenting
name: Wang, Junying
name: Minze, Laurie J.
name: Cox, Timothy C.
name: Li, Xian Chang
name: Xing, Junji
name: Zhang, Zhiqiang
Publisher: name: figshare
Year: 2022
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 1: Table S1. PPM1A is in the TRIM18-binding protein complex. Table S2. The potential ubiquitination sites at the PPM1A molecule. Table S3. Primers for qRT-PCR and PCR used in this study.
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 1039
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 1039, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 1039, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Asymmetric star formation triggered by gas inflow in a barred lenticular galaxy PGC 34107
Creators: name: Lu, Shiying
name: Gu, Qiusheng
name: Ge, Xue
name: Ho, Luis C.
name: Gao, Yulong
name: Chen, Zhengyi
name: Xu, Ke
name: Zhang, Zhi-Yu
name: Shi, Yong
name: Yuan, Qirong
name: Bao, Min
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Comparing to the inactive and gas-poor normal lenticular galaxies (S0s) in the local universe, we study a barred star-forming S0 galaxy, PGC 34107, which has been observed by the Centro Astronómico Hispano Alemán (CAHA) 3.5-m telescope and the Northern Extended Millimeter Array (NOEMA). The spatially resolved ionized gas and molecular gas traced by $^{12}$CO(1-0), hereafter CO(1-0), show the similar distribution and kinematics to the stellar component with an off-center star-forming region, $\sim$380 pc away from the center. The resolved kinematics of molecular CO(1-0) emission reveals that there is a blueshifted (redshifted) velocity component on the receding (approaching) side of the galaxy along the stellar bar. This might provide a plausible evidence of non-circular motion, such as the bar-induced molecular gas inflow. The velocity of molecular gas inflow decreases with approaching towards the peak of the off-center star formation in the north, which might be associated with the inner Lindblad resonance (ILR). In addition to CO(1-0), we also detect the isotopic line of $^{13}$CO(1-0). Most $\rm Hα$, CO(1-0) and $^{13}$CO(1-0) emissions are concentrated on this northern star-forming region. We find that PGC 34107 follows the local stellar mass-metallicity relation, star-forming main sequence, and the Kennicutt-Schmidt law. The resolved and integrated molecular gas main sequence suggest that there is a higher gas fraction in the galaxy central region, which supports a scenario that the bar-induced gas reservoir provides the raw material, and subsequently triggers the central star formation.
description: 18pages, 13figures, 1table, accepted by ApJ
Hyperfine splitting effects in string hadronization
Creators: name: Bierlich, Christian
name: Chakraborty, Smita
name: Gustafson, Gösta
name: Lönnblad, Leif
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We revisit the recipe for hadron formation in the Lund string hadronization model. Given an incoming quark or quark-diquark pair, weights for hadron formation are updated to take hyperfine splitting effects arising from the mass difference between u, d-type and s-type quarks. We find that the procedure improves the description of hadron yields in $\mathrm{e}^+\mathrm{e}^-$ collisions and the $ϕ$ cross section in neutral current DIS. We also show results for proton collisions, and discuss the future use of this study in the context of small system collectivity.
description: 17 pages, 4 figures
Bosonization duality in 2+1 dimensions and critical current correlation functions in Chern-Simons $U(1)\times U(1)$ Abelian Higgs model
Creators: name: Shyta, Vira
name: Nogueira, Flavio S.
name: Brink, Jeroen van den
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: While the phase structure of the $U(1)\times U(1)$-symmetric Higgs theory is still under debate, a version of this theory with an additional Chern-Simons term was recently shown to undergo a second-order phase transition [V. Shyta, J. van den Brink, and F. S. Nogueira, Phys. Rev. Lett. 127, 045701 (2021)]. This theory is dual to a topological field theory of massless fermions featuring two gauge fields. Here we elaborate on several aspects of this duality, focusing on the critical current correlators and on the nature of the critical point as reflected by the bosonization duality. The current correlators associated to the $U(1)\times U(1)$ symmetry and the topological current are shown to coincide up to a universal prefactor, which we find to be the same for both $U(1)$ and $U(1)\times U(1)$ topological Higgs theories. The established duality offers in addition another way to substantiate the claim about the existence of a critical point in the bosonic Chern-Simons $U(1)\times U(1)$ Higgs model: a Schwinger-Dyson analysis of the fermionic dual model shows that no dynamical mass generation occurs. The same cannot be said for the theory without the Chern-Simons term in the action.
description: v2: nearly matches published version; references added
Observation-based modelling of the energetic storm particle event of 14 July 2012
Creators: name: Wijsen, Nicolas
name: Aran, Angels
name: Scolini, Camilla
name: Lario, David
name: Afanasiev, Alexandr
name: Vainio, Rami
name: Sanahuja, Blai
name: Pomoell, Jens
name: Poedts, Stefaan
Publisher: name: arXiv
Year: 2022
Subjects: subject: Space Physics (physics.space-ph)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We model the energetic storm particle (ESP) event of 14 July 2012 using the energetic particle acceleration and transport model named PARADISE, together with the solar wind and coronal mass ejection (CME) model named EUHFORIA. The simulation results illustrate both the capabilities and limitations of the utilised models. We show that the models capture some essential structural features of the ESP event; however, for some aspects the simulations and observations diverge. We describe and, to some extent, assess the sources of errors in the modelling chain of EUHFORIA and PARADISE and discuss how they may be mitigated in the future. The PARADISE model evolves energetic particle distributions in a background solar wind generated by the ideal MHD module of EUHFORIA. The CME generating the ESP event is simulated by using the spheromak model of EUHFORIA, which approximates the CME's flux rope as a linear force-free spheroidal magnetic field. In addition, a tool was developed to trace CME-driven shock waves in the EUHFORIA simulation domain. This tool is used in PARADISE to (i) inject 50 keV protons continuously at the CME-driven shock and (ii) include a foreshock and a sheath region, in which the energetic particle parallel mean free path, $λ_\parallel$, decreases towards the shock wave. The value of $λ_\parallel$ at the shock wave is estimated from in situ observations of the ESP event. For energies below 1 MeV, the simulation results agree well with both the upstream and downstream components of the ESP event observed by the Advanced Composition Explorer (ACE). This suggests that these low-energy protons are mainly the result of interplanetary particle acceleration. In the downstream region, the sharp drop in the energetic particle intensities is reproduced at the entry into the following magnetic cloud, illustrating the importance of a magnetised CME model.
description: 14 pages, 10 figures, accepted for publication in Astronomy & Astrophysics
Commentary on the clinical and preclinical dosage limits of interstitially administered magnetic fluids for therapeutic hyperthermia based on current practice and efficacy models
Creators: name: Southern, Paul
name: Pankhurst, Quentin A.
Publisher: name: Taylor & Francis
Year: 2017
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer

description: We offer a critique of what constitutes a suitable dosage limit, in both clinical and preclinical studies, for interstitially administered magnetic nanoparticles in order to enable therapeutic hyperthermia under the action of an externally applied alternating magnetic field. We approach this first from the perspective of the currently approved clinical dosages of magnetic nanoparticles in the fields of MRI contrast enhancement, sentinel node detection, iron replacement therapy and magnetic thermoablation. We compare this to a simple analytical model of the achievable hyperthermia temperature rise in both humans and animals based on the interstitially administered dose, the heating and dispersion characteristics of the injected fluid, and the strength and frequency of the applied magnetic field. We show that under appropriately chosen conditions a therapeutic temperature rise is achievable in clinically relevant situations. We also show that in such cases it may paradoxically be harder to achieve the same therapeutic temperature rise in a preclinical model. We comment on the implications for the evidence-based translation of hyperthermia based interventions from the laboratory to the clinic.
title: Intersections between Jewish Studies and Habsburg Studies
Creators: name: Corbett, Tim
name: Siegel, Björn
name: Thulin, Mirjam
name: Csáky, Moritz
name: Hödl, Klaus
name: Kasper-Marienberg, Verena
name: Berkovich, Ilya
name: Czakai, Johannes
name: Maślak-Maciejewska, Alicja
name: Stechauner, Martin
name: Dodou, Lida-Maria
name: Heimann-Jelinek, Felicitas
name: Nasr, Omar T.
name: Halbinger, Monika
name: Jánošíková, Magdaléna
name: Keßler, Katrin
name: Kauders, Anthony D.
name: Piskačová, Zora
name: Arnold, Rafael D.
name: Schulz, Michael K.
name: Shapira, Elena
name: Sidky, Sean
name: Sun, Cheuk Him Ryan
name: Tirosh-Samuelson, Hava
name: Tusan, Michelle
name: Weigand, Susanne
Publisher: name: Universitätsverlag Potsdam
Year: 2024
Subjects: subject: 200 Religion

description: In the aftermath of the Shoah and the ostensible triumph of nationalism, it became common in historiography to relegate Jews to the position of the “eternal other” in a series of binaries: Christian/Jewish, Gentile/Jewish, European/Jewish, non-Jewish/Jewish, and so forth. For the longest time, these binaries remained characteristic of Jewish historiography, including in the Central European context. Assuming instead, as the more recent approaches in Habsburg studies do, that pluriculturalism was the basis of common experience in formerly Habsburg Central Europe, and accepting that no single “majority culture” existed, but rather hegemonies were imposed in certain contexts, then the often used binaries are misleading and conceal the complex and sometimes even paradoxical conditions that shaped Jewish life in the region before the Shoah.

The very complexity of Habsburg Central Europe both in synchronic and diachronic perspective precludes any singular historical narrative of “Habsburg Jewry,” and it is not the intention of this volume to offer an overview of “Habsburg Jewish history.” The selected articles in this volume illustrate instead how important it is to reevaluate categories, deconstruct historical narratives, and reconceptualize implemented approaches in specific geographic, temporal, and cultural contexts in order to gain a better understanding of the complex and pluricultural history of the Habsburg Empire and the region as a whole.
description: PaRDeS : Zeitschrift der Vereinigung für Jüdische Studien e.V.; 29
Redshift evolution of the HI detection rate in radio-loud active galactic nuclei
Creators: name: Murthy, Suma
name: Morganti, Raffaella
name: Kanekar, Nissim
name: Oosterloo, Tom
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a search for associated HI 21 cm absorption in a sample of 29 radio-loud active galactic nuclei (AGNs) at $0.7 < z < 1$, carried out with the upgraded Giant Metrewave Radio Telescope. We detect HI 21 cm absorption against none of our target AGNs, obtaining $3σ$ upper limits to the optical depth of $\lesssim$ 1% per 50 km s$^{-1}$ channel. The radio luminosity of our sources is lower than that of most AGNs searched for HI 21 cm absorption at similar redshifts in the literature, and, for all targets except two, the UV luminosity is below the threshold $10^{23}$ W Hz$^{-1}$, above which the HI in the AGN environment has been suggested to be completely ionised. We stacked the HI spectra to obtain a more stringent limit of $\approx 0.17$% per 50 km s$^{-1}$ channel on the average HI 21 cm optical depth of the sample. The sample is dominated by extended radio sources, 24 of which are extended on scales of tens of kiloparsecs. Including similar extended sources at $0.7 < z < 1.0$ from the literature, and comparing with a low-$z$ sample of extended radio sources, we find statistically significant ($\approx 3σ$) evidence that the strength of HI 21 cm absorption towards extended radio sources is weaker at $0.7
description: 15 pages, 6 figures. Accepted for publication in Astronomy & Astrophysics
Lettre de Guillaume-Emmanuel-Joseph de Guilhem de Clermont-Lodève, baron de Sainte-Croix à Jean-François Séguier, 1778-02-28
Creators: name: baron de Sainte-Croix, Guillaume-Emmanuel-Joseph de Guilhem de Clermont-Lodève
name: Guillaume-Emmanuel-Joseph De Guilhem De Clermont-Lodève, Baron De Sainte-Croix
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: Antiquités (général)

description: [transcription] Monsieur et très respectable confrère,

Je remis à Monsieur d'Urre une caisse de livres qu'il m'a promis de vous faire passer par la voie de Monfrin. Elle contient l'ouvrage de Bryant, Antiquit. Reginae, la description du cabinet de Stosch, de magister Athenius et les dissertations grecques d'Hagenbuch que vous avez eu la bonté de me prêter. Je vous en réitère mes remerciements pour le Bryant myth. qui m'appartient. Vous pourrez le lire à votre aise. Vous me rendriez un vrai service de m'apprendre son opinion sur les mystères, et de me faire un court extrait de ce qu'il en dit. Cela me sera fort utile pour l'ouvrage que je compte mettre sous presse l'année prochaine. Je suis actuellement fort occupé à mon édition de l'Ezour Vedam. Cette matière me tourmente étrangement et sans le Père inquisiteur je l'aurais abandonné vingt-fois. La religion et la philosophie des Indiens est un affreux dédale. Les matériaux et les livres originaux nous manquent, quel parti prendre ? donnez moi avis de réception de la caisse et s'il ne vous arrivait pas, écrivez deux mots à Montfrin. Comment se trouve votre santé des temps rigoureux qui nous atatquent ? Soyez persuadé du vif intérêt que je prends à votre conservation et du tendre et inviolable attachement avec lequel j'ai l'honneur d'être, Monsieur, votre très humble et très obéissant serviteur,

Ce 28 février 1778.

Sainte-Croix
description: [personnes citées] Frère Jean-Baptiste Mabil, Louis-François-Laurent d' Urre
description: [reférence bibliographique citée] Hagenbuch, Johann Kaspar, Io. Gasp. Hagenbuchii […] Epistolae epigraphicae ad virum illustrem Ioannem Bovhierium senatus divionensis praesidem; et ad virum celeberrimum Ant. Franc. Gorium […] in qu.
Winckelmann Johann Joachim, Description des pierres gravées de feu le baron Stosch dédiée à feu son Eminence Monseigneur le cardinal Albani, Florence, Bonducci, 1760.. Bryant, Jack, A new system analysis of antient mythology, Londres, 1776
. Haverkamp, Sigebert, Nummophylacium reginae Christinae, quod comprehendit numismata aerea Imperatorum Romanorum, La Haye, 1742.
. Hagenbuch, Caspar, De graecis Thesauri novi Muratoriani Marmoribus quibusdam metricis Diatriba, Zurich, 1744.
description: [lettre editée aussi sur] Maria Stefania Montecalvo (éd.), Guillaume-Emmanuel-Joseph Guilhem de Clermont-Lodève baron de Sainte-Croix (1746-1809). Carteggio e biografia, Florence, Gonnelli, 2014, t. I, p. 98-99.
description: Source: [lieu de Conservation] Nîmes, Bibliothèque Carré d'Art [cote]ms. 141_19, fol. 130
description: Source: ark:/12148/btv1b100152047
Discovery of Three Candidate Magnetar-powered Fast X-ray Transients from Chandra Archival Data
Creators: name: Lin, Dacheng
name: Irwin, Jimmy A.
name: Berger, Edo
name: Nguyen, Ronny
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: It was proposed that a remnant stable magnetar could be formed in a binary neutron-star merger, leading to a fast X-ray transient (FXT) that can last for thousands of seconds. Recently, Xue et al. suggested that CDF-S XT2 was exactly such a kind of source. If confirmed, such emission can be used to search for electromagnetic counterparts to gravitational wave events from binary neutron-star mergers that have short gamma-ray bursts and the corresponding afterglows seen off-axis and thus too weak to be detected. Here we report the discovery of three new FXTs, XRT 170901, XRT 030511, and XRT 110919, from preliminary search over Chandra archival data. Similar to CDF-S XT2, these new FXTs had a very fast rise (less than a few ten seconds) and a plateau of X-ray flux $\sim$$1.0\times10^{-12}$ erg s$^{-1}$ cm$^{-2}$ lasting for 1-2 ks, followed by a steep decay. Their optical/IR counterparts, if present, are very weak, arguing against a stellar flare origin for these FXTs. For XRT 170901, we identified a faint host galaxy with the source at the outskirts, very similar to CDF-S XT2. Therefore, our newly discovered FXTs are also strong candidates for magnetar-powered X-ray transients resulting from binary neutron star mergers.
description: 13 pages, 9 figures, submitted version after addressing the referee's comments