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Hydrodynamics of Young Binaries with Low-Mass Secondaries. / Demidova, T.V.; Grinin, V.P.; Sotnikova, N.Ya.

в: Proceedings of the International Astronomical Union, Том 7, № 282, 2012, стр. 521-524.

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

Harvard

Demidova, TV, Grinin, VP & Sotnikova, NY 2012, 'Hydrodynamics of Young Binaries with Low-Mass Secondaries', Proceedings of the International Astronomical Union, Том. 7, № 282, стр. 521-524. https://doi.org/10.1017/S1743921311028304

APA

Demidova, T. V., Grinin, V. P., & Sotnikova, N. Y. (2012). Hydrodynamics of Young Binaries with Low-Mass Secondaries. Proceedings of the International Astronomical Union, 7(282), 521-524. https://doi.org/10.1017/S1743921311028304

Vancouver

Demidova TV, Grinin VP, Sotnikova NY. Hydrodynamics of Young Binaries with Low-Mass Secondaries. Proceedings of the International Astronomical Union. 2012;7(282):521-524. https://doi.org/10.1017/S1743921311028304

Author

Demidova, T.V. ; Grinin, V.P. ; Sotnikova, N.Ya. / Hydrodynamics of Young Binaries with Low-Mass Secondaries. в: Proceedings of the International Astronomical Union. 2012 ; Том 7, № 282. стр. 521-524.

BibTeX

@article{ce06f7964e27404ebf115a19b4111af9,
title = "Hydrodynamics of Young Binaries with Low-Mass Secondaries",
abstract = "The model of a young star with a low-mass secondary component (q = M2/M1",
keywords = "accretion, accretion discs, hydrodynamics, numerical method, close binaries",
author = "T.V. Demidova and V.P. Grinin and N.Ya. Sotnikova",
year = "2012",
doi = "10.1017/S1743921311028304",
language = "English",
volume = "7",
pages = "521--524",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "282",

}

RIS

TY - JOUR

T1 - Hydrodynamics of Young Binaries with Low-Mass Secondaries

AU - Demidova, T.V.

AU - Grinin, V.P.

AU - Sotnikova, N.Ya.

PY - 2012

Y1 - 2012

N2 - The model of a young star with a low-mass secondary component (q = M2/M1

AB - The model of a young star with a low-mass secondary component (q = M2/M1

KW - accretion

KW - accretion discs

KW - hydrodynamics

KW - numerical method

KW - close binaries

U2 - 10.1017/S1743921311028304

DO - 10.1017/S1743921311028304

M3 - Article

VL - 7

SP - 521

EP - 524

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - 282

ER -

ID: 5400154