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Models of zero-age main sequence stars from 0.15 to 125 solar masses. / Ilin, V. B.

In: Труды астрономической обсерватории ЛГУ. Серия математических наук, Vol. 40, 1985, p. 25-41.

Research output: Contribution to journal › Article

Harvard

Ilin, VB 1985, 'Models of zero-age main sequence stars from 0.15 to 125 solar masses', Труды астрономической обсерватории ЛГУ. Серия математических наук, vol. 40, pp. 25-41. <http://adsabs.harvard.edu/abs/1985TrLen..40...25I>

APA

Ilin, V. B. (1985). Models of zero-age main sequence stars from 0.15 to 125 solar masses. Труды астрономической обсерватории ЛГУ. Серия математических наук, 40, 25-41. http://adsabs.harvard.edu/abs/1985TrLen..40...25I

Vancouver

Ilin VB. Models of zero-age main sequence stars from 0.15 to 125 solar masses. Труды астрономической обсерватории ЛГУ. Серия математических наук. 1985;40:25-41.

Author

Ilin, V. B. / Models of zero-age main sequence stars from 0.15 to 125 solar masses. In: Труды астрономической обсерватории ЛГУ. Серия математических наук. 1985 ; Vol. 40. pp. 25-41.

BibTeX

@article{e4acc30d72f74e37bb82a654105f8f23,
title = "Models of zero-age main sequence stars from 0.15 to 125 solar masses",
abstract = "Chemically homogeneous stellar models (X = 0.70, Y = 0.27, Z = 0.03) in the 0.15-125 solar-mass range are calculated. The structure of the models is examined, and the dependence of the following model parameters on the mass is discussed: luminosity, radius, density, temperature and pressure at the center, gravitational energy, moment of inertia, potential at the center, and effective temperature. The models considered are compared with polytropic and homologous models of chemically homogeneous stars.",
keywords = "Chemical Composition, Main Sequence Stars, Stellar Mass, Stellar Models, Plasma Density, Stellar Luminosity, Stellar Structure, Stellar Temperature",
author = "Ilin, {V. B.}",
year = "1985",
language = "English",
volume = "40",
pages = "25--41",
journal = "Труды астрономической обсерватории ЛГУ. Серия математических наук",

}

RIS

TY - JOUR

T1 - Models of zero-age main sequence stars from 0.15 to 125 solar masses

AU - Ilin, V. B.

PY - 1985

Y1 - 1985

N2 - Chemically homogeneous stellar models (X = 0.70, Y = 0.27, Z = 0.03) in the 0.15-125 solar-mass range are calculated. The structure of the models is examined, and the dependence of the following model parameters on the mass is discussed: luminosity, radius, density, temperature and pressure at the center, gravitational energy, moment of inertia, potential at the center, and effective temperature. The models considered are compared with polytropic and homologous models of chemically homogeneous stars.

AB - Chemically homogeneous stellar models (X = 0.70, Y = 0.27, Z = 0.03) in the 0.15-125 solar-mass range are calculated. The structure of the models is examined, and the dependence of the following model parameters on the mass is discussed: luminosity, radius, density, temperature and pressure at the center, gravitational energy, moment of inertia, potential at the center, and effective temperature. The models considered are compared with polytropic and homologous models of chemically homogeneous stars.

KW - Chemical Composition

KW - Main Sequence Stars

KW - Stellar Mass

KW - Stellar Models

KW - Plasma Density

KW - Stellar Luminosity

KW - Stellar Structure

KW - Stellar Temperature

M3 - Article

VL - 40

SP - 25

EP - 41

JO - Труды астрономической обсерватории ЛГУ. Серия математических наук

JF - Труды астрономической обсерватории ЛГУ. Серия математических наук

ER -

ID: 42891264