Zobrazeno 1 - 10
of 112
pro vyhledávání: '"S. A. Shulman"'
Autor:
R. Y. Lakhin, E. A. Zhirnova, V. V. Shustrov, S. G. Shulman, A. A. Yemelyanov, B. N. Bogomolov
Publikováno v:
Неотложная медицинская помощь, Vol 8, Iss 4, Pp 418-422 (2020)
BACKGROUND. Ultrasound study significantly expanded the possibilities of bedside diagnosis in patients with respiratory failure. Using ultrasound, it is possible to determine the volume of lung damage in the form of collapsed alveoli and infiltration
Externí odkaz:
https://doaj.org/article/0e4c121a2fcb4fe5a2992df6978c3577
Autor:
Vladimir Grinin, S. G. Shulman
Publikováno v:
Astronomy Letters. 45:664-676
The influence of large-scale perturbations in a circumstellar disk on the linear polarization of UX Ori stars is considered. We show that the position angle of the intrinsic linear polarization of a star surrounded by a geometrically thin flared disk
Autor:
Vladimir Grinin, S. G. Shulman
Publikováno v:
Astronomy Letters. 45:384-395
The behavior of the linear polarization parameters of UX Ori stars during their eclipses by circumstellar dust clouds is studied. A circumstellar disk with a disk wind creating a puffing in the dust sublimation zone is considered. We show that the di
Autor:
S G Shulman, V P Grinin
We simulate the polarized radiative transfer in vicinities of the UX Ori type stars during their minima. Our model of an eclipse by an extended disc perturbation generalizes the compact gas-dust cloud eclipse model. We apply the radiative transfer me
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f4a9230a3ea67fbe419ab22181381ffc
Autor:
S. G. Shulman
Publikováno v:
Astrophysics. 60:188-199
The formation of resonance lines in gas flows generated by interactions of circumstellar gas with a star’s magnetosphere is examined. An effective method is proposed for calculating these lines when the magnetospheric wind is highly porous. The res
Autor:
S. G. Shulman
Publikováno v:
Astrophysics. 59:20-30
Possible reasons for the very low projected rotation velocity of BF Ori compared to other UX Ori stars are discussed. The hypothesis of a close companion that slows down the star’s rotation by a tidal interaction is examined. Based on a theory of s
Autor:
G D Havrov, N. V. Sharenkova, S. A. Kazakov, M. A. Grevtsev, S. G. Shulman, M. M. Kazanin, S. M. Solov’ev
Publikováno v:
Journal of Physics: Conference Series. 1697:012183
The experimental data on the thermovoltaic effect in bulk samples of samarium sulfide (SmS) are considered in this work in accordance with the represented kinetic model. The kinetic laws of the elementary process of samarium ions ionization have been
Publikováno v:
Astronomy Letters. 41:407-416
The origin of the blueshifted narrow absorption components in the resonance sodium doublet lines observed in the spectra of some young stars is discussed. Such components are assumed to be formed by the interaction of the circumstellar gas with the s
Autor:
S. G. Shulman
Publikováno v:
Astrophysics. 58:258-275
The shape of spirals formed by the interaction of a circumstellar disk with the magnetosphere in the magnetic propeller regime is examined in the ballistic approximation. The problem is solved analytically. The spirals and their cross sections are il
Publikováno v:
Journal of Occupational and Environmental Hygiene. 1:D107-D111