Standard

An iterative method for constructing stellar systems models: how far does it work? / Sotnikova, Natalia Ya.; Rodionov, Sergei A.

в: Proceedings of the International Astronomical Union, Том 5, № H15, 2009, стр. 203.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Sotnikova, NY & Rodionov, SA 2009, 'An iterative method for constructing stellar systems models: how far does it work?', Proceedings of the International Astronomical Union, Том. 5, № H15, стр. 203. https://doi.org/10.1017/S1743921310008768

APA

Sotnikova, N. Y., & Rodionov, S. A. (2009). An iterative method for constructing stellar systems models: how far does it work? Proceedings of the International Astronomical Union, 5(H15), 203. https://doi.org/10.1017/S1743921310008768

Vancouver

Author

Sotnikova, Natalia Ya. ; Rodionov, Sergei A. / An iterative method for constructing stellar systems models: how far does it work?. в: Proceedings of the International Astronomical Union. 2009 ; Том 5, № H15. стр. 203.

BibTeX

@article{935a2a647c394f30a19e3c5af55adc94,
title = "An iterative method for constructing stellar systems models: how far does it work?",
abstract = "We present a new method for constructing equilibrium phase models for stellar systems. Applications of the iterative method include both modelling of observational data and the construction of initial condition for N-body simulations.",
author = "Sotnikova, {Natalia Ya.} and Rodionov, {Sergei A.}",
year = "2009",
doi = "10.1017/S1743921310008768",
language = "English",
volume = "5",
pages = "203",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "H15",

}

RIS

TY - JOUR

T1 - An iterative method for constructing stellar systems models: how far does it work?

AU - Sotnikova, Natalia Ya.

AU - Rodionov, Sergei A.

PY - 2009

Y1 - 2009

N2 - We present a new method for constructing equilibrium phase models for stellar systems. Applications of the iterative method include both modelling of observational data and the construction of initial condition for N-body simulations.

AB - We present a new method for constructing equilibrium phase models for stellar systems. Applications of the iterative method include both modelling of observational data and the construction of initial condition for N-body simulations.

U2 - 10.1017/S1743921310008768

DO - 10.1017/S1743921310008768

M3 - Article

VL - 5

SP - 203

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - H15

ER -

ID: 5017955