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Planetary Motion in the Atmospheres of Red Giants. / Volobueva, M.I.; Tarakanov, P.A.

в: Astrophysics, 2015, стр. 430-440.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Volobueva, MI & Tarakanov, PA 2015, 'Planetary Motion in the Atmospheres of Red Giants', Astrophysics, стр. 430-440. https://doi.org/10.1007/s10511-015-9396-3

APA

Volobueva, M. I., & Tarakanov, P. A. (2015). Planetary Motion in the Atmospheres of Red Giants. Astrophysics, 430-440. https://doi.org/10.1007/s10511-015-9396-3

Vancouver

Volobueva MI, Tarakanov PA. Planetary Motion in the Atmospheres of Red Giants. Astrophysics. 2015;430-440. https://doi.org/10.1007/s10511-015-9396-3

Author

Volobueva, M.I. ; Tarakanov, P.A. / Planetary Motion in the Atmospheres of Red Giants. в: Astrophysics. 2015 ; стр. 430-440.

BibTeX

@article{02e1ef478fe843d9ab7e7b33abfb4b14,
title = "Planetary Motion in the Atmospheres of Red Giants",
abstract = "{\textcopyright} 2015 Springer Science+Business Media New York When a star reaches the red giant stage in the course of its evolution, its closest planets are in its atmosphere. Numerical gas dynamic models are constructed for hypersonic flow around planets by matter in the atmosphere of a red giant. The results are compared with analytic models for the motion of planets in the atmospheres of stars.",
author = "M.I. Volobueva and P.A. Tarakanov",
year = "2015",
doi = "10.1007/s10511-015-9396-3",
language = "English",
pages = "430--440",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",

}

RIS

TY - JOUR

T1 - Planetary Motion in the Atmospheres of Red Giants

AU - Volobueva, M.I.

AU - Tarakanov, P.A.

PY - 2015

Y1 - 2015

N2 - © 2015 Springer Science+Business Media New York When a star reaches the red giant stage in the course of its evolution, its closest planets are in its atmosphere. Numerical gas dynamic models are constructed for hypersonic flow around planets by matter in the atmosphere of a red giant. The results are compared with analytic models for the motion of planets in the atmospheres of stars.

AB - © 2015 Springer Science+Business Media New York When a star reaches the red giant stage in the course of its evolution, its closest planets are in its atmosphere. Numerical gas dynamic models are constructed for hypersonic flow around planets by matter in the atmosphere of a red giant. The results are compared with analytic models for the motion of planets in the atmospheres of stars.

U2 - 10.1007/s10511-015-9396-3

DO - 10.1007/s10511-015-9396-3

M3 - Article

SP - 430

EP - 440

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

ER -

ID: 3945489