Standard

Wavelets for looking for clumping in the wind of OB stars. / Kholtygin, A.F.

Clumping in hot-star winds : proceedings of an international workshop held in Potsdam, Germany, 18. - 22. June 2007. Potsdam : Universitätsverlag Potsdam, 2008. стр. 248-248.

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференцийстатья в сборнике материалов конференциинаучная

Harvard

Kholtygin, AF 2008, Wavelets for looking for clumping in the wind of OB stars. в Clumping in hot-star winds : proceedings of an international workshop held in Potsdam, Germany, 18. - 22. June 2007. Universitätsverlag Potsdam, Potsdam, стр. 248-248, Clumping in Hot-Star Winds, Potsdam, Германия, 18/06/07. <http://adsabs.harvard.edu/abs/2008cihw.conf..248K>

APA

Kholtygin, A. F. (2008). Wavelets for looking for clumping in the wind of OB stars. в Clumping in hot-star winds : proceedings of an international workshop held in Potsdam, Germany, 18. - 22. June 2007 (стр. 248-248). Universitätsverlag Potsdam. http://adsabs.harvard.edu/abs/2008cihw.conf..248K

Vancouver

Kholtygin AF. Wavelets for looking for clumping in the wind of OB stars. в Clumping in hot-star winds : proceedings of an international workshop held in Potsdam, Germany, 18. - 22. June 2007. Potsdam: Universitätsverlag Potsdam. 2008. стр. 248-248

Author

Kholtygin, A.F. / Wavelets for looking for clumping in the wind of OB stars. Clumping in hot-star winds : proceedings of an international workshop held in Potsdam, Germany, 18. - 22. June 2007. Potsdam : Universitätsverlag Potsdam, 2008. стр. 248-248

BibTeX

@inproceedings{fd8d82adb63f466d88b85448ab598ab7,
title = "Wavelets for looking for clumping in the wind of OB stars",
abstract = "The wind of hot stars are strongly structured and carry the numerous clumps of very differentsizes and masses. Contrary to the Wolf-Rayet stars, the individual clumps in the winds of OBstars are rather small and not very long-lived objects. This makes the detecting clumps in OBstar wind a hard problem. We use the wavelet analysis as a powerful tool for searching thedetails of the line profiles, connected with clumps. We use the dynamical wavelet spectra ofline profile variations (lpv) for studying a regular and a stochastic lpv.",
author = "A.F. Kholtygin",
year = "2008",
language = "English",
isbn = "978-3-940793-33-1",
pages = "248--248",
booktitle = "Clumping in hot-star winds",
publisher = "Universit{\"a}tsverlag Potsdam",
address = "Germany",
note = "Clumping in Hot-Star Winds : International Workshop held in Potsdam ; Conference date: 18-06-2007 Through 22-06-2007",

}

RIS

TY - GEN

T1 - Wavelets for looking for clumping in the wind of OB stars

AU - Kholtygin, A.F.

PY - 2008

Y1 - 2008

N2 - The wind of hot stars are strongly structured and carry the numerous clumps of very differentsizes and masses. Contrary to the Wolf-Rayet stars, the individual clumps in the winds of OBstars are rather small and not very long-lived objects. This makes the detecting clumps in OBstar wind a hard problem. We use the wavelet analysis as a powerful tool for searching thedetails of the line profiles, connected with clumps. We use the dynamical wavelet spectra ofline profile variations (lpv) for studying a regular and a stochastic lpv.

AB - The wind of hot stars are strongly structured and carry the numerous clumps of very differentsizes and masses. Contrary to the Wolf-Rayet stars, the individual clumps in the winds of OBstars are rather small and not very long-lived objects. This makes the detecting clumps in OBstar wind a hard problem. We use the wavelet analysis as a powerful tool for searching thedetails of the line profiles, connected with clumps. We use the dynamical wavelet spectra ofline profile variations (lpv) for studying a regular and a stochastic lpv.

UR - https://d-nb.info/1218791012/34

M3 - Conference contribution

SN - 978-3-940793-33-1

SP - 248

EP - 248

BT - Clumping in hot-star winds

PB - Universitätsverlag Potsdam

CY - Potsdam

T2 - Clumping in Hot-Star Winds

Y2 - 18 June 2007 through 22 June 2007

ER -

ID: 4487989