cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¼Ð°ÑÐ¾Ð², Ð­Ð´ÑÐ°ÑÐ´
name: ÐÐ²ÑÐ°ÑÐ¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2009
Subjects: Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²Ñ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 Â«ÐÐ½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ°Ð»ÑÐ½ÑÐ¼Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸ÑÐ¼Ð¸, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð·Ð°ÑÑÐ°Ñ Ð¿Ð¾ ÑÐ°Ð·Ð°Ð¼ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð¼ÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»ÑÐ½ÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹, ÑÑÐµÑ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐ¸ÑÐºÐ° Ð¿ÑÐ¸ Ð¾ÑÐµÐ½ÐºÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð², Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð², Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð²Ð½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸ÐµÐ¹ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð²ÑÑÑÐµÐ¹ ÑÐºÐ¾Ð»Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 080500 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ».
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Nucleation of superconductivity and vortex matter in superconductor - ferromagnet hybrids
Creators: name: Aladyshkin, A. Yu.
name: Silhanek, A. V.
name: Gillijns, W.
name: Moshchalkov, V. V.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The theoretical and experimental results concerning the thermodynamical and low-frequency transport properties of hybrid structures, consisting of spatially-separated conventional low-temperature superconductor (S) and ferromagnet (F), is reviewed. Since the superconducting and ferromagnetic parts are assumed to be electrically insulated, no proximity effect is present and thus the interaction between both subsystems is through their respective magnetic stray fields. Depending on the temperature range and the value of the external field H_{ext}, different behavior of such S/F hybrids is anticipated. Rather close to the superconducting phase transition line, when the superconducting state is only weakly developed, the magnetization of the ferromagnet is solely determined by the magnetic history of the system and it is not influenced by the field generated by the supercurrents. In contrast to that, the nonuniform magnetic field pattern, induced by the ferromagnet, strongly affect the nucleation of superconductivity leading to an exotic dependence of the critical temperature T_{c} on H_{ext}. Deeper in the superconducting state the effect of the screening currents cannot be neglected anymore. In this region of the phase diagram various aspects of the interaction between vortices and magnetic inhomogeneities are discussed. In the last section we briefly summarize the physics of S/F hybrids when the magnetization of the ferromagnet is no longer fixed but can change under the influence of the superconducting currents. As a consequence, the superconductor and ferromagnet become truly coupled and the equilibrium configuration of this "soft" S/F hybrids requires rearrangements of both, superconducting and ferromagnetic characteristics, as compared with "hard" S/F structures.
description: Topical review, submitted to Supercond. Sci. Tech., 67 pages, 33 figures, 439 references
Unifying devices in A tale of a tub
Creators: name: Clark, Richard David
Publisher: name: University of British Columbia
Year: 2011

description: One of the major problems for readers and students of A Tale of a Tub is its apparent lack of internal unity and coherence. Faced with a welter of seemingly contradictory and inconsistent arguments and attitudes, reader and student alike have frequently been forced to concede defeat and turn to Swift's "more profitable" works for consolation. The purpose of the present study has been to indicate the existence, in the Tale, of numerous unifying devices, a recognition of which may enable the reader to perceive and appreciate the essential unity and coherence of an admittedly complex literary entity. Emphasis has been primarily upon the "dramatic impact" of the Tale, and the contribution of images and themes to this impact. Classification of images and themes has been made in terms of the definitions offered in the text. Persuasive oratory is the instrument to achievement in the Tubbian world, and it is with the motives and methods of Tubbian orators that the study is primarily concerned. The pervasive themes of the mechanical operation of the spirit and madness are among the unifying devices in the Tale. The first seven chapters are devoted to an exploration of images, devices, and thematic developments as unifying devices. Four subsequent chapters discuss the relationships between elements in the Tale and certain of the cultural dissentions of which these elements provide reflections. There has been no attempt at inclusiveness in the selection of representative cultural elements. Rather, in the selection of materials from Hobbes, Dryden, Wycherley, Sprat, the Cambridge Platonists, Glanvill, and Shaftesbury, the attempt has been only to indicate the major preoccupations of the age. Where obvious similarities exist between attitudes, as they do between the attitudes of Hobbes and those of the scientific virtuosi, the emphasis is upon Swift's capacity to make fine distinctions between similar attitudes and to indicate these distinctions in his methods of attack. Conversely, the inclusion of apparently disparate "philosophies," such as those of Hobbes and Shaftesbury, is intended to demonstrate Swift's ability to comprehend in one attack a great variety of disparate attitudes. It has been found necessary, in the interests of clarity, to include a certain amount of explanation and elaboration of materials relative to the cultural background. The conclusion of the study is primarily concerned with the reader's reaction to the "dramatic impact" of the Tale. Certain of Swift's "satiric criteria" or norms are tentatively offered for consideration. These are such as may be readily available to the reader from a careful examination of the text and an exploration of his own reaction to the text.
Finding large average submatrices in high dimensional data
Creators: name: Shabalin, Andrey A.
name: Weigman, Victor J.
name: Perou, Charles M.
name: Nobel, Andrew B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Genomics (q-bio.GN)
subject: Quantitative Methods (q-bio.QM)
subject: FOS: Biological sciences

description: The search for sample-variable associations is an important problem in the exploratory analysis of high dimensional data. Biclustering methods search for sample-variable associations in the form of distinguished submatrices of the data matrix. (The rows and columns of a submatrix need not be contiguous.) In this paper we propose and evaluate a statistically motivated biclustering procedure (LAS) that finds large average submatrices within a given real-valued data matrix. The procedure operates in an iterative-residual fashion, and is driven by a Bonferroni-based significance score that effectively trades off between submatrix size and average value. We examine the performance and potential utility of LAS, and compare it with a number of existing methods, through an extensive three-part validation study using two gene expression datasets. The validation study examines quantitative properties of biclusters, biological and clinical assessments using auxiliary information, and classification of disease subtypes using bicluster membership. In addition, we carry out a simulation study to assess the effectiveness and noise sensitivity of the LAS search procedure. These results suggest that LAS is an effective exploratory tool for the discovery of biologically relevant structures in high dimensional data. Software is available at https://genome.unc.edu/las/.
description: Published in at http://dx.doi.org/10.1214/09-AOAS239 the Annals of Applied Statistics (http://www.imstat.org/aoas/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Scalar mesons in $η'\to3π^{0},π^{0}π^{+}π^{-}$ decays
Creators: name: Likhoded, A. K.
name: Luchinsky, A. V.
name: Samoylenko, V. D.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The decays $η'\to3π^{0}$ and $π^{0}π^{+}π^{-}$ were consider in isobar model approach. Branching ratio and Dalitz-plot shape of the decay $η'\to3π^{0}$ can be explain by $a0$- and $σ$-meson contributions. The $σ$ meson term is needed for the Dalitz-plot distribution reconstruction. The branching ratio of the decay $η'\to π^{0}π^{+}π^{-}$ can be calculated in the same isobar framework. The prediction for the Dalitz-plot of this decay is shown which strongly dependents from model parameters.
description: 10 pages, 6 figures
The cosmology dependence of weak lensing cluster counts
Creators: name: Marian, Laura
name: Smith, Robert E.
name: Bernstein, Gary M.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the main results of a numerical study of weak lensing cluster counting. We examine the scaling with cosmology of the projected-density-peak mass function. Our main conclusion is that the projected-peak and the three-dimensional mass functions scale with cosmology in an astonishingly close way. This means that, despite being derived from a two-dimensional field, the weak lensing cluster abundance can be used to constrain cosmology in the same way as the three-dimensional mass function probed by other types of surveys.
description: 4 pages, 2 figures. Accepted for publication in ApJL. Figure 1 modified, unchanged conclusions
Physical structure and water line spectrum predictions of the Intermediate Mass protostar OMC2-FIR4
Creators: name: Crimier, N.
name: Ceccarelli, C.
name: Lefloch, B.
name: Faure, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Aims. Intermediate Mass (IM) stars are an important component of our Galaxy, as they significantly contribute to the interstellar FUV field and, consequently, play an important role in the energy balance of the ISM. Despite their importance, very little is known about their formation process and only a few studies have been devoted to characterize the first phases in the evolution of intermediate mass protostars. Here we consider in great detail the case of the brightest and closest known young IM protostar: FIR4 in the OMC2 component of the Orion molecular cloud complex. Methods. We analyzed the available continuum emission (maps and SED) through one-dimensional dust radiative transfer calculations. We ran large grids of models to find the envelope model that best fits the data. The derived dust density and temperature profiles have been then used to compute the gas temperature profile, equating gas cooling and heating terms across the envelope. Last, we computed the water line spectrum for various possible values of water abundance. Results. The luminosity of FIR4 has been reevaluated to 1000 Lo, making FIR4 definitively an Intermediate Mass protostar. The envelope surrounding FIR4 has a relatively shallow density power law index, ~ 0.6. The most surprising result is that the gas and dust are thermally decoupled in the interior of the envelope, where the dust ices sublimate at 100 K. This has important consequences in the interpretation of the line data. We provide the predictions for the water spectrum, and discuss in detail the lines which will be observed by the Herschel Space Observatory .
description: 14 pages and 14 figures. A&A, accepted
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð·Ð¾Ð²ÑÑ ÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐ¸Ð¹ Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ¸Ð¸ Ð»Ð¸ÐºÐ²Ð¸Ð´ÑÑÐ° ÑÑÐµÑ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Fe-Sn-S
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¥Ð°ÑÐ»Ð°Ð½Ð¾Ð²Ð°, ÐÐ»ÑÐ³Ð°
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: 2016
Subjects: ÑÐ°Ð·Ð¾Ð²ÑÐµ ÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐ¸Ñ
ÑÑÐµÑ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð¶ÐµÐ»ÐµÐ·Ð¾-Ð¾Ð»Ð¾Ð²Ð¾-ÑÐµÑÐ°
Ð¿Ð¾Ð²ÐµÑÑ Ð½Ð¾ÑÑÐ¸ Ð»Ð¸ÐºÐ²Ð¸Ð´ÑÑÐ°
Ð¿Ð¸ÑÐ¾Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ð¸ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ÑÐ»ÑÐ¶Ð¸Ð»Ð° ÑÑÐµÑÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð¶ÐµÐ»ÐµÐ·Ð¾-Ð¾Ð»Ð¾Ð²Ð¾-ÑÐµÑÐ°, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÑÑÐ°ÑÑÑ Ð»ÐµÑÑÑÐµÑÑÑÑ Ð¸ Ð°Ð³ÑÐµÑÑÐ¸Ð²Ð½Ð¾ÑÑÑÑ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð².ÐÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð»Ð¾ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ¸Ð¸ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸ Ð»Ð¸ÐºÐ²Ð¸Ð´ÑÑÐ° Ð½Ð¸Ð·ÐºÐ¾ÑÐµÑÐ½Ð¸ÑÑÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ, Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐµÐ²Ð´Ð¾Ð±Ð¸Ð½Ð°ÑÐ½ÑÐ¼ ÑÐµÑÐµÐ½Ð¸ÐµÐ¼ FeS-SnS.
An examination of the social structure of the women's unit, Oakalla Prison Farm
Creators: name: Coutts, Dorothy Mae
Publisher: name: University of British Columbia
Year: 2011

description: This is an examination of the social structure of a women's prison. The prison has five primary tasks: custody, internal order, self-maintenance, punishment and reformation. Verbal priority is given to reformation, but custody and internal order take precedence in actual practice. Matrons prefer to play their roles in different ways. Those who subscribe to a habit-forming philosophy of reformation prefer working on the morning shift. Their views and practices are in harmony with the requirements of custody. Those who subscribe to a basic-change philosophy prefer the more relaxed and permissive atmosphere of the afternoon shift. Their views and practices are frequently in conflict with the requirements of custody. And structural pressure tends to force these matrons to become more custodial over time. In exchange for obedience and conformity in some spheres the matrons agree not to tamper with the attitudes and values of the inmates. This bargain for compliance seems essential given the present social structure of the prison. The inmates suffer from the deprivation of liberty, goods and services, heterosexual relationships, autonomy, security and, at the Women's Unit, privacy. The addicts and "rounders" adopt cohesive modes of response to these deprivations. "Squealers", "hack lovers" and "part players" adopt alienative modes of response. The inmates differ by groups in their characteristic responses to official oppression. The younger addict groups rebel habitually, the older groups conform overtly but do not change their basic values.
Additional file 2 of Assessing the suitability of general practice electronic health records for clinical prediction model development: a data quality assessment
Creators: name: Thuraisingam, Sharmala
name: Chondros, Patty
name: Dowsey, Michelle M.
name: Spelman, Tim
name: Garies, Stephanie
name: Choong, Peter F.
name: Gunn, Jane
name: Manski-Nankervis, Jo-Anne
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Additional file 2: Data linkage methodology.
Radio and optical orientations of galaxies
Creators: name: Battye, R. A.
name: Browne, I. W. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the correlations between optical and radio isophotal position angles for 14302 SDSS galaxies with $r$ magnitudes brighter than 18 and which have been associated with extended FIRST radio sources. We identify two separate populations of galaxies using the colour, concentration and their principal components. Surprisingly strong statistical alignments are found: late-type galaxies are overwhelmingly biased towards a position angle differences of $0^{\circ}$ and early-type galaxies to $90^{\circ}$. The late-type alignment can be easily understood in terms of the standard picture in which the radio emission is intimately related to areas of recent star-formation. In early-type galaxies the radio emission is expected to be driven by accretion on to a nuclear black hole. We argue that the observed correlation of the radio axis with the minor axis of the large-scale stellar distribution gives a fundamental insight into the structure of elliptical galaxies, for example, whether or not the nuclear kinematics are decoupled form the rest of the galaxy. Our results imply that the galaxies are oblate spheroids with their radio emission aligned with the minor axis. Remarkably the strength of the correlation of the radio major axis with the optical minor axis depends on radio loudness. Those objects with a low ratio of FIRST radio flux density to total stellar light show a strong minor axis correlation while the stronger radio sources do not. This may reflect different formation histories for the different objects and we suggest we may be seeing the different behaviour of rationally supported and non-rotationally supported ellipticals.
description: Version to appear in MNRAS
Quantum Fusion of Strings (Flux Tubes) and Domain Walls
Creators: name: Bolognesi, S.
name: Shifman, M.
name: Voloshin, M. B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider formation of composite strings and domain walls as a result of fusion of two elementary objects (elementary strings in the first case and elementary walls in the second) located at a distance from each other. The tension of the composite object T_2 is assumed to be less than twice the tension of the elementary object T_1, so that bound states are possible. If in the initial state the distance d between the fusing strings or walls is much larger than their thickness and satisfies the conditions T_1 d^2 >> 1 (in the string case) and T_1 d^3 >> 1 (in the wall case), the problem can be fully solved quasiclassically. The fusion probability is determined by the first, "under the barrier" stage of the process. We find the bounce configuration and its extremal action S_B. In the wall problem e^{-S_B} gives the fusion probability per unit time per unit area. In the string case, due to a logarithmic infrared divergence, the problem is well formulated only for finite-length strings. The fusion probability per unit time can be found in the limit in which the string length is much larger than the distance between two merging strings.
description: 24 pages, 10 figures; v2: ref added
Adaptive asymptotically efficient estimation in heteroscedastic nonparametric regression
Creators: name: Galtchouk, Leonid
name: Pergamenchtchikov, Serguei
Publisher: name: arXiv
Year: 2010
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics
subject: 62G08

description: The paper deals with asymptotic properties of the adaptive procedure proposed in the author paper, 2007, for estimating an unknown nonparametric regression. %\cite{GaPe1}. We prove that this procedure is asymptotically efficient for a quadratic risk, i.e. the asymptotic quadratic risk for this procedure coincides with the Pinsker constant which gives a sharp lower bound for the quadratic risk over all possible estimates
Magnetic Fields from Heterotic Cosmic Strings
Creators: name: Gwyn, Rhiannon
name: Alexander, Stephon
name: Brandenberger, Robert H.
name: Dasgupta, Keshav
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Large-scale magnetic fields are observed today to be coherent on galactic scales. While there exists an explanation for their amplification and their specific configuration in spiral galaxies -- the dynamo mechanism -- a satisfying explanation for the original seed fields required is still lacking. Cosmic strings are compelling candidates because of their scaling properties, which would guarantee the coherence on cosmological scales of any resultant magnetic fields at the time of galaxy formation. We present a mechanism for the production of primordial seed magnetic fields from heterotic cosmic strings arising from M theory. More specifically, we make use of heterotic cosmic strings stemming from M5--branes wrapped around four of the compact internal dimensions. These objects are stable on cosmological time scales and carry charged zero modes. Therefore a scaling solution of such defects will generate seed magnetic fields which are coherent on galactic scales today.
description: 19 pages, 2 .eps figures, PRD format
Additional file 4 of CDKN2AIP is critical for spermiogenesis and germ cell development
Creators: name: Cao, Yuming
name: Sun, Qi
name: Chen, Zhenlie
name: Lu, Jing
name: Geng, Ting
name: Ma, Ling
name: Zhang, Yuanzhen
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 4: Figure S4. Principle and data analysis process of RNA Seq and IP-MS. (A) The details of experimental operation and data analysis of RNA seq. (B) The details of experimental operation and data analysis of IP-MS.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð²ÑÐ°ÑÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ ÐºÐ»Ð°ÑÑÐ° NP ÑÐµÐ¾ÑÐ¸Ð¸ Ð³ÑÐ°ÑÐ¾Ð²
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¤ÐµÐ´Ð¾ÑÐ¾Ð², ÐÐ²Ð°Ð½
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Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ
ÐÑÐ°ÑÐ¾Ð² ÑÐµÐ¾ÑÐ¸Ñ
Ð³Ð°Ð¼Ð¸Ð»ÑÑÐ¾Ð½Ð¾Ð²Ñ ÑÐ¸ÐºÐ»Ñ

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ: Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° Lizhi Du, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐµÐ³Ð¾ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ Ð¿ÑÐ¸ ÑÐµÑÐµÐ½Ð¸Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¿Ð¾Ð¸ÑÐºÐ° Ð³Ð°Ð¼Ð¸Ð»ÑÑÐ¾Ð½Ð¾Ð²Ð° ÑÐ¸ÐºÐ»Ð° Ð² Ð½ÐµÐ¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð³ÑÐ°ÑÐ°Ñ. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸Ð´ÐµÐ¹, Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Lizhi Du, Ð±ÑÐ» Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾ ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¿Ð¾Ð¸ÑÐºÐ° Ð³Ð°Ð¼Ð¸Ð»ÑÑÐ¾Ð½Ð¾Ð²Ð° ÑÐ¸ÐºÐ»Ð° Ð² Ð½ÐµÐ¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð³ÑÐ°ÑÐ°Ñ. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¹ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð±ÑÐ»Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ, Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ¶Ð´Ð°ÑÑÐ¸Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð°.
Ionized Gas in the Smith Cloud
Creators: name: Hill, Alex S.
name: Haffner, L. Matthew
name: Reynolds, Ronald J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present Wisconsin H-Alpha Mapper observations of ionized gas in the Smith Cloud, a high velocity cloud which Lockman et al. have recently suggested is interacting with the Galactic disk. Our H-alpha map shows the brightest H-alpha emission, 0.43 \pm 0.04 R, coincident with the brightest H I, while slightly fainter H-alpha emission (0.25 \pm 0.02 R) is observed in a region with H I intensities < 0.1 times as bright as the brightest H I. We derive an ionized mass of \gtrsim 3 \times 10^6 M_\odot, comparable to the H I mass, with the H^+ mass spread over a considerably larger area than the H I. An estimated Galactic extinction correction could adjust these values upwards by 40 %. H-alpha and [S II] line widths towards the region of brightest emission constrain the electron temperature of the gas to be between 8000 K and 23000 K. A detection of [N II] λ6583 in the same direction with a line ratio [N II] / H-alpha = 0.32 \pm 0.05 constrains the metallicity of the cloud: for typical photoionization temperatures of 8000-12000 K, the nitrogen abundance is 0.15-0.44 times solar. These results lend further support to the claim that the Smith Cloud is new material accreting onto the Galaxy.
description: 8 pages, 4 figures, ApJ accepted. This is the ApJ version of work presented in an early form as Hill et al 2009a (arxiv:0901.0712)
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð¸ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÐ¾Ð»Ð¾Ð²Ð¾Ð¹ Ð½Ð° 150 Ð¼ÐµÑÑ Ð² Ð³. Ð§ÐµÑÐµÐ¿Ð¾Ð²ÐµÑ
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¸Ð½ÑÐµÐ²Ð°, ÐÐ°Ñ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: 2018
Subjects: Ð´Ð¸ÐµÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÑÐ¾Ð»Ð¾Ð²Ð°Ñ
ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð¼ÐµÐ½Ñ
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Ð¿ÑÐ¸ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐµ, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
Additional file 2 of Non-alcoholic fatty liver is associated with increased risk of irritable bowel syndrome: a prospective cohort study
Creators: name: Wu, Shanshan
name: Yuan, Changzheng
name: Yang, Zhirong
name: Liu, Si
name: Zhang, Qian
name: Zhang, Shutian
name: Zhu, Shengtao
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Mental Health

description: Additional file 2. FigureS1. Restricted cubic splinefor the association of baseline fatty liver index with incident IBS. Figure S2. Risk of incident IBSassociated with NAFLD type (lean, non-obese and obese NAFLD).
title: Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð°Ñ Ð¸Ð½ÑÐµÑÐ¿ÑÐµÑÐ°ÑÐ¸Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¼ÑÑÐ»Ð¾Ð² Ð¾Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ¿Ð¾ÑÑÐ°
title: Modern interpretation of the socio-political meanings of olympic sports
Creators: name: ÐÑÐ±ÑÑÐµÐ²Ð°, ÐÑÐ´Ð¼Ð¸Ð»Ð°
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ Ð¾Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¾Ðµ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ
ÑÐµÐ½Ð½Ð¾ÑÑÐ¸
Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾ÑÐµÑÐ¸Ñ
ÑÑÑÐ´ÐµÐ½ÑÑ
Ð°Ð½ÐºÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
modern Olympic movement
values
contradictions
students
questionnaire

description: ÐÐ¾ÑÑÐµÐ´ÑÑÐ²Ð¾Ð¼ ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð¿ÑÐ¾ÑÐ° 2838 ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² 28ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÑ Ð²ÑÐ·Ð¾Ð² Ð¸ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ¾Ð² Ð¿Ð¾Ð»ÑÑÐµÐ½Ð° ÑÑÐ±ÑÐµÐºÑÐ¸Ð²Ð½Ð°Ñ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð¸ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¹ Ð¸Ñ Ð¿ÑÐ¾ÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ Ð¾Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¾Ð¼ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ð¸, Ðº Ð³Ð»Ð°Ð²Ð½ÑÐ¼ Ð¸Ð· ÐºÐ¾ÑÐ¾ÑÑÑ Ð¾ÑÐ½Ð¾ÑÑÑÑÑ: ÑÑÐ°Ð½ÑÐ³ÐµÐ½Ð´ÐµÑÐ½Ð¾ÑÑÑ, Ð´Ð¸ÑÐºÑÐ¸Ð¼Ð¸Ð½Ð°ÑÐ¸Ñ Ð¿Ð¾ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¼Ñ Ð¿ÑÐ¸Ð·Ð½Ð°ÐºÑ, Ð²Ð¾ÐµÐ½Ð½ÑÐµ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÑ, ÑÑÐ¸ÑÐ¸Ð¹Ð½ÑÐµ Ð±ÐµÐ´ÑÑÐ²Ð¸Ñ, ÑÐ¿Ð¸Ð´ÐµÐ¼Ð¸Ð¸, ÑÐµÑÑÐ¾ÑÐ¸Ð·Ð¼, Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ°ÑÐ°ÐºÑÐµÑÐ°. ÐÑÐ¼ÐµÑÐ°ÐµÑÑÑ, ÑÑÐ¾ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ¿Ð¾ÑÑÐ° Ð Ð¾ÑÑÐ¸Ð¸, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð² Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ Ð½Ð°ÑÐ¾Ð´Ð¸ÑÑÑ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¸, Ð²Ð¸Ð´ÑÑÑÑ Ð² ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ð¸ Ð´ÑÑÐ¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÐºÐ»Ð°ÑÑÐµÑÐ°, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð½Ð° Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ð¸, Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð¿ÑÐ¸ ÑÐ¼ÐµÑÐµÐ½Ð¸Ð¸ ÑÐµÐ½ÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¸Ð¼ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸ÐµÐ¼ Ð² ÑÑÐ¾ÑÐ¾Ð½Ñ Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾Ð»ÑÑÐ½Ð¾Ð³Ð¾ Ð¼Ð¸ÑÐ°.
description: Through a sociological survey of 2838 students of 28 sports universities and faculties, a subjective assessment of socio-political problems and trends in their manifestation in the modern Olympic movement was obtained, the main of which include: transgenderism, discrimination based on nationality, military conflicts, natural disasters, epidemics, terrorism, organizational problems. It is noted that the prospects for the development of Olympic sports in Russia, which is currently in political isolation, are seen in the creation of a friendly international cluster based on mutual understanding, mutual assistance while shifting the control center of the Olympic movement towards a multipolar world.
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð² Ð±ÑÐ´Ð¶ÐµÑÐ½Ð¾Ð¼ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ð¸ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ·ÑÐ¼Ð¸Ð½, ÐÐ¸ÑÐ¸Ð»Ð»
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: Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ðµ
Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð±ÑÐ´Ð¶ÐµÑ
ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ
ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°

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title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹ ÑÐµÑÐ¸ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð¾Ð² ÑÐ²ÐµÐ¹Ð½ÑÑ Ð¿ÑÐ¸Ð½Ð°Ð´Ð»ÐµÐ¶Ð½Ð¾ÑÑÐµÐ¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÑÐ¾ÑÐ¸Ð½Ð°, ÐÐ½Ð°ÑÑÐ°Ñ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: 2016
Subjects: Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸
ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ñ
ÑÐ¸Ð½ÐµÑÐ³Ð¸Ñ
ÑÐ²ÐµÐ¹Ð½ÑÐµ Ð¿ÑÐ¸Ð½Ð°Ð´Ð»ÐµÐ¶Ð½Ð¾ÑÑÐ¸
integrated marketing communications
advertising company
synergy
sewing supplies

description: Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹ ÑÐµÑÐ¸ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð¾Ð² ÑÐ²ÐµÐ¹Ð½ÑÑ Ð¿ÑÐ¸Ð½Ð°Ð´Ð»ÐµÐ¶Ð½Ð¾ÑÑÐµÐ¹. ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: ÑÐµÑÑ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð¾Ð² ÑÐ²ÐµÐ¹Ð½ÑÑ Ð¿ÑÐ¸Ð½Ð°Ð´Ð»ÐµÐ¶Ð½Ð¾ÑÑÐµÐ¹ Â«ÐÐ¸Ñ ÑÐ¸ÑÑÑÂ». ÐÐ°Ð´Ð°ÑÐ¸: ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ ÐÐÐ; Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð²Ð¸Ð´Ñ ÐÐÐ; Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹; Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð°Ñ ÑÑÐµÐ´Ð° ÑÐµÑÐ¸ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð¾Ð² ÑÐ²ÐµÐ¹Ð½ÑÑ Ð¿ÑÐ¸Ð½Ð°Ð´Ð»ÐµÐ¶Ð½Ð¾ÑÑÐµÐ¹ Â«ÐÐ¸Ñ ÑÐ¸ÑÑÑÂ»; ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ°Ð¿Ñ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ; Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ.
description: Research purpose: development of campaign of integrated marketing communications of a retail network of sewing accessories. Object of research: retail network of sewing accessories "World of sewing". Tasks: concept IMÐ¡ is considered; types of IMÐ¡ are defined; features of development of campaign of integrated marketing communications are revealed; the marketing environment of a retail network of sewing accessories "The world of sewing" is analyzed; the main stages of campaign IMÐ¡ are developed; campaign IMÐ¡ efficiency evaluation is made.
title: Ð¡Ð¿ÐµÑÐ¸ÑÐ¸ÐºÐ° Ð½ÐµÐ¾Ð»Ð¾Ð³Ð¸Ð·Ð¼Ð¾Ð² Ð² ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¼ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð´Ð¸ÑÐºÑÑÑÐµ (Ð½Ð° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ðµ Ð³Ð°Ð·ÐµÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÐºÐ¾ÑÐ¿ÑÑÐ° ÐÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾ÑÐ¿ÑÑÐ° ÑÑÑÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°)
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ÑÐ½Ð¸Ð½Ð°, ÐÐ»ÑÐ³Ð°
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: Ð½ÐµÐ¾Ð»Ð¾Ð³Ð¸Ð·Ð¼Ñ
ÐÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¹ ÐºÐ¾ÑÐ¿ÑÑ ÑÑÑÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° Ð½ÐµÐ¾Ð»Ð¾Ð³Ð¸Ð·Ð¼Ð¾Ð² Ð² Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð´Ð¸ÑÐºÑÑÑÐµ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð³Ð°Ð·ÐµÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÐºÐ¾ÑÐ¿ÑÑÐ° ÐÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾ÑÐ¿ÑÑÐ° ÑÑÑÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°. ÐÐ°Ð½Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¾ Ð½ÐµÐ¾Ð»Ð¾Ð³Ð¸Ð·Ð¼Ð°Ñ Ð¸ Ð¸Ñ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸ÑÑ, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¸ÑÑÐ¾ÑÐ¸Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð½ÐµÐ¾Ð»Ð¾Ð³Ð¸Ð·Ð¼Ð¾Ð² Ð² ÑÑÑÑÐºÐ¾Ð¼ ÑÐ·ÑÐºÐµ Ð¸ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð´Ð¸ÑÐºÑÑÑÐ°. ÐÐ½Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÑÑ ÐºÐ¾Ð½ÑÐµÐºÑÑÑÐ°Ð»ÑÐ½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½ÐµÐ¾Ð»Ð¾Ð³Ð¸Ð·Ð¼Ð¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¿Ð¾Ð¸ÑÐºÐ° Ð² ÐºÐ¾ÑÐ¿ÑÑÐµ.
title: ÐÐ°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð¾ ÐºÑÐµÐ´Ð¸ÑÐ½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ½Ð¸ÑÐ¾Ð²Ð°, ÐÐ²Ð³ÐµÐ½Ð¸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: 2017
Subjects: Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð½ÐµÑÐ¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
ÐºÑÐµÐ´Ð¸ÑÐ½ÑÐµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
Ð¾ÑÐµÐ½ÐºÐ° Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð°

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°ÑÐ¸ÐºÐ¸ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð° ÐºÑÐµÐ´Ð¸ÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ, ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ Ð¸ Ð¿ÑÐ¸Ð·Ð½Ð°ÐºÐ¸ Ð½ÐµÑÐ¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹; Ð½ÐµÑÐ¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ (Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð¾) ÐºÑÐµÐ´Ð¸ÑÐ½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð½ÐµÑÐ¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ (Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð°) ÐºÑÐµÐ´Ð¸ÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹. Ð Ð°ÑÐºÑÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¸ Ð¿ÑÐ¸Ð·Ð½Ð°ÐºÐ¸ Ð½ÐµÑÐ¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ (Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð°) ÐºÑÐµÐ´Ð¸ÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹, Ð¼ÐµÑÑ Ð¿Ð¾ Ð¿ÑÐµÐ´ÑÐ¿ÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð° ÐÐ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÐµÐ»Ð¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð° ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ñ Ð±Ð°Ð½ÐºÐ¾Ð² (ÐÐÐ Â«ÐÐÐ Â«ÐÐ¸ÐºÐ¸Ð½Ð³Â» Ð¸ ÐÐ Â«ÐÐ ÐÂ» (ÐÐÐ)). ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð° Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼ÑÑ Ð±Ð°Ð½ÐºÐ¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¨ÐµÐ¼ÐµÑÐµÐ²Ð° Ð.Ð.
title: Ð Ð¸ÑÐºÐ¸ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð¿ÑÐ¸ Ð½Ð¸Ð·ÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¾Ð¿Ð»Ð°ÑÐµ ÑÑÑÐ´Ð° ÑÐ°Ð±Ð¾ÑÐ¸Ñ
title: Risks in the economy of construction with low productivity and wages of workers
Creators: name: ÐÑÐ´Ð·Ð¸Ð½Ð¾Ð², ÐÐ°ÑÐ¸Ð»Ð¸Ð¹
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ ÑÐµÑÐµÐ½Ð¸Ñ (Ð ÐÐ¡ÐâÐ­â2022)", Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼ (8; 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ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÑÑÐ´Ð°
ÑÐ°ÑÐ¸ÑÐ½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°
ÑÐ´ÐµÐ»ÑÐ½Ð°Ñ ÑÐ°ÑÑÐµÐ½ÐºÐ°
Ð·Ð°ÑÐ°Ð±Ð¾ÑÐ½Ð°Ñ Ð¿Ð»Ð°ÑÐ°
ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¹ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»
ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¶Ð¸Ð·Ð½Ð¸
tariff system
piece rate
wages
human capital
quality of life

description: ÐÐ»Ð°Ð²Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð¾Ð¹ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµ Ð Ð¾ÑÑÐ¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐ´Ð°. ÐÐ¸Ð½Ð°Ð¼Ð¸ÐºÐ° Ð·Ð°ÑÐ°Ð±Ð¾ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑ Ð½Ð°ÑÐ¾Ð´Ð¸ÑÑÑ Ð² Ð¿ÑÑÐ¼Ð¾Ð¹ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ ÑÑÐ¾Ð²Ð½Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐ´Ð°. ÐÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÑÑÐ´Ð° Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð´Ð¾Ð»Ð¶Ð½Ð° ÑÐ°ÑÑÐ¸ Ð½Ðµ Ð½Ð¸Ð¶Ðµ 5% Ð² Ð³Ð¾Ð´, ÑÑÐ¾Ð±Ñ Ð²ÑÐ¹ÑÐ¸ Ð½Ð° ÑÑÐ¾Ð²ÐµÐ½Ñ Ð²ÐµÐ´ÑÑÐ¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸Ðº Ð¼Ð¸ÑÐ°. Ð 2020 Ð³. ÑÑÐ¾Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ñ ÑÐ¾ÑÑÐ°Ð²Ð¸Ð» Ð²ÑÐµÐ³Ð¾ 1,4%. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐ¾ÑÑÐ° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐ´Ð° Ð¸ ÐµÐ³Ð¾ Ð¾Ð¿Ð»Ð°ÑÑ Ð² Ð¾Ð´Ð½Ð¾Ð¹ Ð¸Ð· Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐ¸Ñ Ð¾ÑÑÐ°ÑÐ»ÐµÐ¹ Ð½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²Ð° â ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ðµ.
description: The main problem in the Russian economy is the growth of labor productivity. The dynamics of wages is in direct proportion to the level of labor productivity. Labor productivity in Russia must grow at least 5% per year in order to reach the level of the world's leading economies. In 2020, this figure was only 1.4%. This article examines the problems of growth in labor productivity and remuneration in one of the most important sectors of the national economy - construction.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÑÑÐ° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½ÑÑ ÑÐ°ÑÑÐ»Ð¾Ð²
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°Ð¶Ð¸Ð½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´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: ÐÐ¾Ð³Ð¸ÑÑÐ¸ÐºÐ°
Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½ÑÐ¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑ
Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½ÑÐ¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½ÑÐµ ÑÐ°ÑÑÐ»Ñ, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÐ¹ Ð¿ÑÐ¸Ð²Ð¾Ð·Ð¾Ðº
Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð³Ð¾ÑÐ¾Ð²Ð½Ð¾ÑÑÐ¸ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾Ð¾Ð±ÑÐµÑÑÐ²Ð° Ð¸ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸, Ð² Ð»Ð¸ÑÐµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹ Ð¸ ÑÑÐ´Ð¾Ð²ÑÑ Ð³ÑÐ°Ð¶Ð´Ð°Ð½, Ðº Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ° Ð¸ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½ÑÑ ÑÐ°ÑÑÐ»Ð¾Ð² Ð² Ð¿ÐµÑÐµÐ²Ð¾Ð·ÐºÐ¸ ÑÐ¾Ð²Ð°ÑÐ¾Ð² Ð¸ Ð¿Ð¾Ð²ÑÐµÐ´Ð½ÐµÐ²Ð½ÑÑ Ð¶Ð¸Ð·Ð½Ñ.
 ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÐ½ÐºÐ° Ð³ÑÑÐ·Ð¾Ð¿ÐµÑÐµÐ²Ð¾Ð·Ð¾Ðº Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ½ÐºÐ¸ Ð¸ ÑÑÑÐ°Ð½Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð³Ð¾ÑÐ¾Ð²ÑÐµ Ðº Ð¿Ð¾ÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°.
 ÐÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð½Ð¾Ð²Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°.
ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð² Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼ Ð²Ð¾Ð¿ÑÐ¾ÑÐµ Ð¸ Ð²Ð¾Ð¿ÑÐ¾ÑÐµ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ.
Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð²ÑÐ³Ð¾Ð´Ð° Ð¾Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð´Ð»Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹.
Hadronic transport approach to neutrino nucleus scattering: the Giessen BUU model and its validation
Creators: name: Leitner, T.
name: Buss, O.
name: Mosel, U.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We present the GiBUU model for neutrino nucleus scattering: assuming impulse approximation, this reaction is treated as a two step process. In the initial state step, the neutrinos interact with bound nucleons. In the final state step, the outgoing particles of the initial reaction are propagated through the nucleus and undergo final state interactions. In this contribution, we focus on the validation of the initial and final state interaction treatment in GiBUU using experimental data for pion-nucleus, photon-nucleus and electron-nucleus scattering.
description: To appear in the proceedings of 45th Winter School in Theoretical Physics 'Neutrino Interactions: from Theory to Monte Carlo Simulations', Ladek-Zdroj, Poland, Feb. 2009
Ovarian dysgerminoma with torsion
Creators: name: Sulthana, Parveen
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Genital / Reproductive system female
subject: MR
subject: Diagnostic procedure
subject: Neoplasia

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 21 years
description: Clinical History: A 21 year old female patient presented with pain in the right iliac fossa for past 1 week. She had regular menstrual periods. No history of vomiting. Final Diagnosis: Malignant germ cell tumor(Dysgerminoma) from right ovary with torsion
Additional file 6 of CDKN2AIP is critical for spermiogenesis and germ cell development
Creators: name: Cao, Yuming
name: Sun, Qi
name: Chen, Zhenlie
name: Lu, Jing
name: Geng, Ting
name: Ma, Ling
name: Zhang, Yuanzhen
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 6: Table S1. Primer sequences are used in this study.
title: Ð¡Ð¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð¾ÑÑÐµÑÐºÐ¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²
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¸ÑÐ¾Ð½ÑÐµÐ²Ð°, Ð¢Ð°ÑÑÑ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: 2018
Subjects: ÑÐ²Ð¾ÑÑÐµÑÐºÐ°Ñ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·
Ð²Ð¾Ð»Ð¾Ð½ÑÐµÑÑÑÐ²Ð¾
Ð½Ð°ÑÑÐ½ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÑÑÐ½Ð¾ÑÑÑ Ð¸ ÑÐ°ÐºÑÐ¾ÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð¾ÑÑÐµÑÐºÐ¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐµÑÐºÐ¾Ð¹ Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð¸. ÐÐ°Ð½Ð¾ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ ÑÐ²Ð¾ÑÑÐµÑÐºÐ¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÐµÐµ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ðµ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¸Ð´Ñ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸ ÑÐ²Ð¾ÑÑÐµÑÐºÐ¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð² ÐÐ£ÐÐµ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ Ð·Ð° ÑÑÐ±ÐµÐ¶Ð¾Ð¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð¾ÑÑÐµÑÐºÐ¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸.
Optical Images of an Exosolar Planet 25 Light Years from Earth
Creators: name: Kalas, Paul
name: Graham, James R.
name: Chiang, Eugene
name: Fitzgerald, Michael P.
name: Clampin, Mark
name: Kite, Edwin S.
name: Stapelfeldt, Karl
name: Marois, Christian
name: Krist, John
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Fomalhaut is a bright star 7.7 parsecs (25 light years) from Earth that harbors a belt of cold dust with a structure consistent with gravitational sculpting by an orbiting planet. Here, we present optical observations of an exoplanet candidate, Fomalhaut b. In the plane of the belt, Fomalhaut b lies approximately 119 astronomical units (AU) from the star and 18 AU from the belt, matching predictions. We detect counterclockwise orbital motion using Hubble Space Telescope observations separated by 1.73 years. Dynamical models of the interaction between the planet and the belt indicate that the planet's mass is at most three times that of Jupiter for the belt to avoid gravitational disruption. The flux detected at 800 nm is also consistent with that of a planet with mass no greater than a few times that of Jupiter. The brightness at 600 nm and the lack of detection at longer wavelengths suggest that the detected flux may include starlight reflected off a circumplanetary disk, with dimension comparable to the orbits of the Galilean satellites. We also observed variability of unknown origin at 600 nm.
description: 25 pages; 4 tables; 4 figures. Science, November 13, 2008