Standard
Stochastic clump model of hot star winds. / Kholtygin, AF.
THERMAL AND IONIZATION ASPECTS OF FLOWS FROM HOT STARS: OBSERVATIONS AND THEORY. ed. / HJG Lamers; A Sapar. Astronomical Society of the Pacific, 2000. p. 231-232 (ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES; Vol. 204).
Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Research
Harvard
Kholtygin, AF 2000,
Stochastic clump model of hot star winds. in HJG Lamers & A Sapar (eds),
THERMAL AND IONIZATION ASPECTS OF FLOWS FROM HOT STARS: OBSERVATIONS AND THEORY. ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES, vol. 204, Astronomical Society of the Pacific, pp. 231-232, Workshop on Thermal and Ionization Aspects of Flows from Hot Stars - Observations and Theory, TARTU, Estonia,
23/08/99.
APA
Kholtygin, AF. (2000).
Stochastic clump model of hot star winds. In HJG. Lamers, & A. Sapar (Eds.),
THERMAL AND IONIZATION ASPECTS OF FLOWS FROM HOT STARS: OBSERVATIONS AND THEORY (pp. 231-232). (ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES; Vol. 204). Astronomical Society of the Pacific.
Vancouver
Kholtygin AF.
Stochastic clump model of hot star winds. In Lamers HJG, Sapar A, editors, THERMAL AND IONIZATION ASPECTS OF FLOWS FROM HOT STARS: OBSERVATIONS AND THEORY. Astronomical Society of the Pacific. 2000. p. 231-232. (ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES).
Author
Kholtygin, AF. /
Stochastic clump model of hot star winds. THERMAL AND IONIZATION ASPECTS OF FLOWS FROM HOT STARS: OBSERVATIONS AND THEORY. editor / HJG Lamers ; A Sapar. Astronomical Society of the Pacific, 2000. pp. 231-232 (ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES).
BibTeX
@inproceedings{36cb4a6c712a4cf38e947c4dd223f3c0,
title = "Stochastic clump model of hot star winds",
abstract = "The stochastic clump model of the winds of early-type stars based on the clump model of the wind is proposed. The formation of the inhomogeneities (clumps) in this model is considered as a stochastic process. The model is well suited both to obtain the mean line profile, which is very close to the observed one, and to reproduce an amplitude and a common pattern of the line profile variability in the spectra of the Wolf-Rayet and OB stars.",
keywords = "RAYET",
author = "AF Kholtygin",
year = "2000",
language = "Английский",
isbn = "1-58381-031-5",
series = "ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES",
publisher = "Astronomical Society of the Pacific",
pages = "231--232",
editor = "HJG Lamers and A Sapar",
booktitle = "THERMAL AND IONIZATION ASPECTS OF FLOWS FROM HOT STARS: OBSERVATIONS AND THEORY",
address = "Соединенные Штаты Америки",
note = "null ; Conference date: 23-08-1999 Through 27-08-1999",
}
RIS
TY - GEN
T1 - Stochastic clump model of hot star winds
AU - Kholtygin, AF
PY - 2000
Y1 - 2000
N2 - The stochastic clump model of the winds of early-type stars based on the clump model of the wind is proposed. The formation of the inhomogeneities (clumps) in this model is considered as a stochastic process. The model is well suited both to obtain the mean line profile, which is very close to the observed one, and to reproduce an amplitude and a common pattern of the line profile variability in the spectra of the Wolf-Rayet and OB stars.
AB - The stochastic clump model of the winds of early-type stars based on the clump model of the wind is proposed. The formation of the inhomogeneities (clumps) in this model is considered as a stochastic process. The model is well suited both to obtain the mean line profile, which is very close to the observed one, and to reproduce an amplitude and a common pattern of the line profile variability in the spectra of the Wolf-Rayet and OB stars.
KW - RAYET
M3 - статья в сборнике материалов конференции
SN - 1-58381-031-5
T3 - ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES
SP - 231
EP - 232
BT - THERMAL AND IONIZATION ASPECTS OF FLOWS FROM HOT STARS: OBSERVATIONS AND THEORY
A2 - Lamers, HJG
A2 - Sapar, A
PB - Astronomical Society of the Pacific
Y2 - 23 August 1999 through 27 August 1999
ER -
