Spectrophotometry of V711 Tauri

dc.contributor.author	Joshi, S. C.
dc.contributor.author	Srivastava, R. K.
dc.contributor.author	Srivastava, J. B.
dc.date.accessioned	2010-02-16T05:44:57Z
dc.date.available	2010-02-16T05:44:57Z
dc.date.issued	1989
dc.identifier.citation	This article is downloaded from ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/520
dc.description.abstract	SPectrophotometric observations of the RS CVn binary system V711 Tau (HR 1099), covering the wavelength interval λλ3300-7100 Å, have been presented. A comparision of the standard spectral scans of V711 Tau with the spectral scans of the stars of known spectral types and luminosity classes taken from the Breger (1976) catalogue shows that, at all phases shown in the diagram, the spectral-luminosity type of the star is K0IV of K0III. The magnitude of the system fluctuates from 5.ͫ71 to 5.ͫ79 average being 5.ͫ75 approximately, the faintest being near 0.ᴾ43 and the brightest near 0.ᴾ78. The region around Balmer jump and near Hα region is apparently variable.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass152-85
dc.subject	RS CVn, V711 Tau (HR 1099)	en_US
dc.title	Spectrophotometry of V711 Tauri	en_US
dc.type	Article	en_US