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Large-scale Wind Structures in OB Supergiants: a Search for Rotationally Modulated Hα variability

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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


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