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Evolution of Angular Momentum Distribution in Exoplanet Systems. / Tarakanov, P.A.; Artamonov, A.S.

In: Astrophysics, Vol. 58, No. 4, 2015, p. 550-566.

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

Harvard

Tarakanov, PA & Artamonov, AS 2015, 'Evolution of Angular Momentum Distribution in Exoplanet Systems', Astrophysics, vol. 58, no. 4, pp. 550-566. https://doi.org/10.1007/s10511-015-9407-4

APA

Tarakanov, P. A., & Artamonov, A. S. (2015). Evolution of Angular Momentum Distribution in Exoplanet Systems. Astrophysics, 58(4), 550-566. https://doi.org/10.1007/s10511-015-9407-4

Vancouver

Tarakanov PA, Artamonov AS. Evolution of Angular Momentum Distribution in Exoplanet Systems. Astrophysics. 2015;58(4):550-566. https://doi.org/10.1007/s10511-015-9407-4

Author

Tarakanov, P.A. ; Artamonov, A.S. / Evolution of Angular Momentum Distribution in Exoplanet Systems. In: Astrophysics. 2015 ; Vol. 58, No. 4. pp. 550-566.

BibTeX

@article{f5d16f9386a0420291526f4dceb1e8bf,
title = "Evolution of Angular Momentum Distribution in Exoplanet Systems",
abstract = "The distribution of angular momentum is investigated in {"}star-planet systems, taking due account of stellar evolution effects. Numerical simulation is carried out for 15 systems for which stellar rotation data are available. Consideration of changes in stellar structure is confirmed to be significant for the evolution of momentum distribution. A conclusion is drawn regarding reduction of dispersion for values of the ratio of the star's orbital angular momentum to its rotational angular momentum resulting from evolution.",
author = "P.A. Tarakanov and A.S. Artamonov",
year = "2015",
doi = "10.1007/s10511-015-9407-4",
language = "English",
volume = "58",
pages = "550--566",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "4",

}

RIS

TY - JOUR

T1 - Evolution of Angular Momentum Distribution in Exoplanet Systems

AU - Tarakanov, P.A.

AU - Artamonov, A.S.

PY - 2015

Y1 - 2015

N2 - The distribution of angular momentum is investigated in "star-planet systems, taking due account of stellar evolution effects. Numerical simulation is carried out for 15 systems for which stellar rotation data are available. Consideration of changes in stellar structure is confirmed to be significant for the evolution of momentum distribution. A conclusion is drawn regarding reduction of dispersion for values of the ratio of the star's orbital angular momentum to its rotational angular momentum resulting from evolution.

AB - The distribution of angular momentum is investigated in "star-planet systems, taking due account of stellar evolution effects. Numerical simulation is carried out for 15 systems for which stellar rotation data are available. Consideration of changes in stellar structure is confirmed to be significant for the evolution of momentum distribution. A conclusion is drawn regarding reduction of dispersion for values of the ratio of the star's orbital angular momentum to its rotational angular momentum resulting from evolution.

U2 - 10.1007/s10511-015-9407-4

DO - 10.1007/s10511-015-9407-4

M3 - Article

VL - 58

SP - 550

EP - 566

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 4

ER -

ID: 3987651