dc.contributor.author |
Morel, T |
|
dc.contributor.author |
Marchenko, S. V |
|
dc.contributor.author |
Pati, A. K |
|
dc.contributor.author |
Kuppuswamy, K |
|
dc.contributor.author |
Carini, M. T |
|
dc.contributor.author |
Wood, E |
|
dc.contributor.author |
Zimmerman, R |
|
dc.date.accessioned |
2008-10-15T12:22:04Z |
|
dc.date.available |
2008-10-15T12:22:04Z |
|
dc.date.issued |
2004-06 |
|
dc.identifier.citation |
Monthly Notices of the Royal Astronomical Society, Vol. 351, No. 2, pp. 552 - 568 |
en |
dc.identifier.issn |
0035-8711 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3943 |
|
dc.description.abstract |
We present the results of a long-term monitoring campaign of the Hα line in a sample of bright OB supergiants (O7.5-B9) which aims at detecting rotationally modulated changes potentially related to the existence of large-scale wind structures. A total of 22 objects were monitored during 36 nights spread over six months in 2001-2002. Coordinated broad-band photometric observations were also obtained for some targets. Conspicuous evidence for variability in Hα is found for the stars displaying a feature contaminated by wind emission. Most changes take place on a daily time-scale, although hourly variations are also occasionally detected. Convincing evidence for a cyclical pattern of variability in Hα has been found in two stars: HD 14134 and HD 42087. Periodic signals are also detected in other stars, but independent confirmation is required. Rotational modulation is suggested from the similarity between the observed recurrence time-scales (in the range 13-25 d) and estimated periods of stellar rotation. We call attention to the atypical case of HD 14134, which exhibits a clear 12.8-d periodicity, both in the photometric and in the spectroscopic data sets. This places this object among a handful of early-type stars where one may observe a clear link between extended wind structures and photospheric disturbances. Further modelling may test the hypothesis that azimuthally-extended wind streams are responsible for the patterns of spectral variability in our target stars. |
en |
dc.language.iso |
en |
en |
dc.publisher |
The Royal Astronomical Society |
en |
dc.relation.uri |
http://fr.arxiv.org/abs/astro-ph/0403155 |
en |
dc.relation.uri |
http://dx.doi.org/10.1111/j.1365-2966.2004.07799.x |
en |
dc.subject |
Stars: Early-Type |
en |
dc.subject |
Stars: Emission-Line |
en |
dc.subject |
Be |
en |
dc.subject |
Stars: Rotation |
en |
dc.subject |
Supergiants |
en |
dc.subject |
Stars: Winds |
en |
dc.subject |
Outflows |
en |
dc.title |
Large-scale wind structures in OB supergiants: a search for rotationally modulated Hα variability |
en |
dc.type |
Article |
en |