Spectroscopic state of the Be Star ζ Tauri in 1976-1986

dc.contributor.author	Mon, M.
dc.contributor.author	Kogure, T.
dc.contributor.author	Suzuki, M.
dc.contributor.author	Singh, M.
dc.date.accessioned	2010-01-18T05:40:26Z
dc.date.available	2010-01-18T05:40:26Z
dc.date.issued	1992
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/441
dc.description.abstract	The long-term variations of the radial velocities (RV) of the shell absorption lines and the violet-to-red ratio (V/R) of the emission double peaks of ζ Tau are examined, based on spectrograms taken at the Okayama, Astrophysical Observatory. It is found that the pscudo-periodic variation was terminated around 1982 and that ζ Tau seems to have entered a new quiet phase in its long-term activity.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	pasj44-73
dc.subject	Be stars, ζ Tau – line profile, V/R – radial velocity	en_US
dc.title	Spectroscopic state of the Be Star ζ Tauri in 1976-1986	en_US
dc.type	Article	en_US