Distribution of absolute of bright Be stars in Pleiades

dc.contributor.author	Goraya, P. S.
dc.date.accessioned	2010-03-10T06:55:16Z
dc.date.available	2010-03-10T06:55:16Z
dc.date.issued	1984
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/629
dc.description.abstract	We present newly measured energy distribution from λλ3200-7500Å of five late-type Be stars in Pleiades cluster for search of peculiarities of Be stars continuum energy distributions. Empirical effective temperatures of Be stars have been derived by comparing observed and computed fluxes in the visible region. The variation of the flux in the Balmer continuum region of Pleione (28 Tau) has been discussed.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass105-323
dc.subject	Be stars, Pleisdes cluster	en_US
dc.title	Distribution of absolute of bright Be stars in Pleiades	en_US
dc.type	Article	en_US