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

In: Astrophysics, Vol. 58, No. 3, 2015, p. 430-440.

Research output: Contribution to journal › Article › peer-review

Harvard

Volobueva, MI & Tarakanov, PA 2015, 'Planetary Motion in the Athmospheres of Red Giants', Astrophysics, vol. 58, no. 3, pp. 430-440. <http://link.springer.com/article/10.1007/s10511-015-9396-3?wt_mc=internal.event.1.SEM.ArticleAuthorOnlineFirst>

APA

Volobueva, M. I., & Tarakanov, P. A. (2015). Planetary Motion in the Athmospheres of Red Giants. Astrophysics, 58(3), 430-440. http://link.springer.com/article/10.1007/s10511-015-9396-3?wt_mc=internal.event.1.SEM.ArticleAuthorOnlineFirst

Vancouver

Volobueva MI, Tarakanov PA. Planetary Motion in the Athmospheres of Red Giants. Astrophysics. 2015;58(3):430-440.

Author

Volobueva, M.I. ; Tarakanov, P. A. / Planetary Motion in the Athmospheres of Red Giants. In: Astrophysics. 2015 ; Vol. 58, No. 3. pp. 430-440.

BibTeX

@article{166c359d7dff4b15a1bba9ac529d67a0,
title = "Planetary Motion in the Athmospheres of Red Giants",
abstract = "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.",
keywords = "red giants: extrasolar planets",
author = "M.I. Volobueva and Tarakanov, {P. A.}",
year = "2015",
language = "English",
volume = "58",
pages = "430--440",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "3",

}

RIS

TY - JOUR

T1 - Planetary Motion in the Athmospheres of Red Giants

AU - Volobueva, M.I.

AU - Tarakanov, P. A.

PY - 2015

Y1 - 2015

N2 - 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 - 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.

KW - red giants: extrasolar planets

M3 - Article

VL - 58

SP - 430

EP - 440

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 3

ER -

ID: 5784013