Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Yu. K. Ananjevskaja"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:3962-3971
We consider optically thin spherical stellar envelopes with dipole magnetic field. The source of magnetic dipole field is assumed point like and emits the non-polarized monochromatic radiation. This paper carry on the previous paper of authors, where
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d49b5ee7eea3eb8253c9d5f9890588d8
https://doi.org/10.1093/mnras/stad805
https://doi.org/10.1093/mnras/stad805
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 514:3685-3691
We consider optically thin spherical stellar envelopes with dipole magnetic field. The source of magnetic dipole field is assumed a star with radius Rs and magnetic moment $\boldsymbol{ M}$. We also assume that a star emits the non-polarized radiatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::995420b2b10d69f4addccd772722c11c
https://doi.org/10.1093/mnras/stac1553
https://doi.org/10.1093/mnras/stac1553
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 512:2707-2715
We consider the semi-infinite plane-parallel electron atmosphere with chaotic magnetic field B′ ≤ 1010 G, when the parameter $x^{\prime 2}=(\omega _{B^{\prime }}/\omega)^2 \simeq 0.87 \times 10^{-16}\lambda ^2(\mu \mathrm{ m}) B^{\prime 2}(G)$ ca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b979b44701e5bd50655e91816ee48682
https://doi.org/10.1093/mnras/stac700
https://doi.org/10.1093/mnras/stac700
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 506:4805-4818
We derive the radiative transfer equations for all Stokes parameters of continuum radiation in atmospheres with any value of homogeneous magnetic field $\boldsymbol{B}$. The explicit formulas for cross-sections and the phase shifts are given with all
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::74e8efad255c4bdc9b2e27008198cdf7
https://doi.org/10.1093/mnras/stab2020
https://doi.org/10.1093/mnras/stab2020
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 499:1499-1505
We consider the emission of resonance line radiation from rotating circular accretion disc with the progressive increasing height (the inclined ring). Our theory can also be applied to the rotating spot-like sources of resonance radiation. We assume
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::19a6f915598b8b04a4f62d9d5d63f069
https://doi.org/10.1093/mnras/staa2964
https://doi.org/10.1093/mnras/staa2964
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 496:4108-4114
We consider the influence of absorbing dust particles on the intensity and polarization of radiation in chaotically magnetized atmospheres. The Milne problem is considered. It is known that the existence of absorbing dust particles leads to more elon
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::63c424dbf178d888bc2e7ff87c0a40a4
https://doi.org/10.1093/mnras/staa1357
https://doi.org/10.1093/mnras/staa1357
Autor:
E. Jilinski, Natalia A. Drake, Alexander F. Kholtygin, J. Telting, Yu. K. Ananjevskaja, M. A. Pogodin, A. Herrera, C. B. Pereira, G. A. Galazutdinov
Publikováno v:
Astrophysics. 62:183-201
High-resolution spectroscopic data for the binary system HD83058 located in the OB association Sco-Cen are presented. The observations were made at the ESO and Sierra Armazones (Chile) observatories over 3 seasons: in March 1998, in 2007-2009, and in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::edde4b913c9451aafd6bcff2465b24f7
https://doi.org/10.1007/s10511-019-09573-8
https://doi.org/10.1007/s10511-019-09573-8
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 486:885-893
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b0566f7863047dfdb0e14deaa3f08686
https://doi.org/10.1093/mnras/stz917
https://doi.org/10.1093/mnras/stz917
We study the resonance line emission from the rotating plane optically thick accretion disc, consisting of free electrons and resonant atoms. We use the standard assumption that the source of continuum radiation is located near central plane of the a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa221059511e0806885f3b8a0b88154e
http://arxiv.org/abs/1907.06416
http://arxiv.org/abs/1907.06416
We consider the influence of Faraday rotation in chaotic magnetic field on the intensity and linear polarization of multiple scattered radiation. All fluctuations are assumed as Gaussian type and isotropic. The values of magnetic field are less than
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20490ba00769aceb3893f5d6c3bfd5e8