| 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.date.accessioned | 2008-06-05T12:11:59Z | |
| dc.date.available | 2008-06-05T12:11:59Z | |
| dc.date.issued | 2003 | |
| dc.identifier.citation | BASI, Vol. 31, No. 3&4, pp. 333 - 335 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/2409 | |
| dc.description.abstract | We present preliminary results of a long-term spectroscopic monitoring of a sample of bright OB-supergiants aimed at establishing the incidence of co-rotating, large-scale wind structures by detecting rotationally modulated variability in H. Dramatic line-profile variations operating on a daily (and in some cases on a hourly) timescale are observed. A detailed period analysis has been so far carried out for 2 stars, and revealed in both cases the existence of cyclical H variations consistent with rotational modulation. In the case of HD 14134, the same periodicity is found in the contemporaneous light curve | en |
| dc.format.extent | 84940 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of India | en |
| dc.relation.uri | http://adsabs.harvard.edu/abs/2003BASI...31..333M | en |
| dc.subject | Stars: early-type | en |
| dc.subject | Stars: supergiants | en |
| dc.subject | Stars: emmision-line | en |
| dc.subject | Stars: winds | en |
| dc.subject | Outflows | en |
| dc.subject | Stars: rotation | en |
| dc.subject | stars: individual | en |
| dc.subject | HD 14134 | en |
| dc.subject | HD 24912 | en |
| dc.title | Large-scale Wind Structures in OB Supergiants: a Search for Rotationally Modulated Hα variability | en |
| dc.type | Article | en |