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Line Profile microvariability and wind structure for OB stars. / Kholtygin, A.F.; Fabrika, S.N.; Sudnik, N.P.

In: PROCEEDINGS OF SYMPOSIA OF THE INTERNATIONAL ASTRONOMICAL UNION, Vol. 6, No. Symp. S272, 2010, p. 200-201.

Research output: Contribution to journal › Article

Harvard

Kholtygin, AF, Fabrika, SN & Sudnik, NP 2010, 'Line Profile microvariability and wind structure for OB stars', PROCEEDINGS OF SYMPOSIA OF THE INTERNATIONAL ASTRONOMICAL UNION, vol. 6, no. Symp. S272, pp. 200-201. https://doi.org/10.1017/S1743921311010337

APA

Kholtygin, A. F., Fabrika, S. N., & Sudnik, N. P. (2010). Line Profile microvariability and wind structure for OB stars. PROCEEDINGS OF SYMPOSIA OF THE INTERNATIONAL ASTRONOMICAL UNION, 6(Symp. S272), 200-201. https://doi.org/10.1017/S1743921311010337

Vancouver

Kholtygin AF, Fabrika SN, Sudnik NP. Line Profile microvariability and wind structure for OB stars. PROCEEDINGS OF SYMPOSIA OF THE INTERNATIONAL ASTRONOMICAL UNION. 2010;6(Symp. S272):200-201. https://doi.org/10.1017/S1743921311010337

Author

Kholtygin, A.F. ; Fabrika, S.N. ; Sudnik, N.P. / Line Profile microvariability and wind structure for OB stars. In: PROCEEDINGS OF SYMPOSIA OF THE INTERNATIONAL ASTRONOMICAL UNION. 2010 ; Vol. 6, No. Symp. S272. pp. 200-201.

BibTeX

@article{546d8a2c2a764de8b78b0472c53c903f,
title = "Line Profile microvariability and wind structure for OB stars",
abstract = "We report the results of searching for the line profile variability (lpv) in the spectra of OB stars. The wavelets were used for looking for the irregular lpv in the spectra of program stars. We connect the appearance of irregular details in the lpv with the formation and destruction the small-scale substructures (clumps) in the wind.",
keywords = "OB stars, variability, line profiles",
author = "A.F. Kholtygin and S.N. Fabrika and N.P. Sudnik",
year = "2010",
doi = "10.1017/S1743921311010337",
language = "English",
volume = "6",
pages = "200--201",
journal = "Symposium (International Astronomical Union)",
issn = "0074-1809",
publisher = "Springer Nature",
number = "Symp. S272",

}

RIS

TY - JOUR

T1 - Line Profile microvariability and wind structure for OB stars

AU - Kholtygin, A.F.

AU - Fabrika, S.N.

AU - Sudnik, N.P.

PY - 2010

Y1 - 2010

N2 - We report the results of searching for the line profile variability (lpv) in the spectra of OB stars. The wavelets were used for looking for the irregular lpv in the spectra of program stars. We connect the appearance of irregular details in the lpv with the formation and destruction the small-scale substructures (clumps) in the wind.

AB - We report the results of searching for the line profile variability (lpv) in the spectra of OB stars. The wavelets were used for looking for the irregular lpv in the spectra of program stars. We connect the appearance of irregular details in the lpv with the formation and destruction the small-scale substructures (clumps) in the wind.

KW - OB stars

KW - variability

KW - line profiles

U2 - 10.1017/S1743921311010337

DO - 10.1017/S1743921311010337

M3 - Article

VL - 6

SP - 200

EP - 201

JO - Symposium (International Astronomical Union)

JF - Symposium (International Astronomical Union)

SN - 0074-1809

IS - Symp. S272

ER -

ID: 5218699