On the shell star pleione (BU Tauri)

dc.contributor.author	Ojha, D. K.
dc.contributor.author	Joshi, S. C.
dc.date.accessioned	2010-01-19T08:34:53Z
dc.date.available	2010-01-19T08:34:53Z
dc.date.issued	1991
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/457
dc.description.abstract	BU Tauri (Pleione) an interesting star in the Pleiades cluster, has been observed spectrophotometrically. The energy distribution curves of the star have been discussed vis a vis model atmospheres for normal stars in the appropriate range of temperature and effective gravity. The changes in the energy distribution curve noticed during our observations and previous observations taken from the literature have been pointed out. On the basis of the measured Hα emission equivalent width, a rough estimate of the dimensions of the extended envelop of the star has been made.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	jaa12-213
dc.subject	Be star, Energy distribution	en_US
dc.title	On the shell star pleione (BU Tauri)	en_US
dc.type	Article	en_US