Spectrophotometry of AR Lacertae

dc.contributor.author	Chaubey, U. S.
dc.contributor.author	Singh, M.
dc.date.accessioned	2010-02-01T06:04:36Z
dc.date.available	2010-02-01T06:04:36Z
dc.date.issued	1990
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/476
dc.description.abstract	Spectrum scans of the RS CVn-type eclipsing binary star AR Lac at different phases in the wavelength range λλ3200-7600 Å taken through Hilger and Watts monochromator equipped with 104-cm telescope of Uttar Pradesh State Observatory, Naini Tal, have been presented and discussed. By subtracting the reduced fluxes of the spectrum scan obtained during the totality of the primary eclipse from the fluxes of the spectrum scans obtained outside the eclipse, the continuum energy distribution data of the primary star of AR Lac have been derived.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass166-177
dc.subject	AR Lac	en_US
dc.title	Spectrophotometry of AR Lacertae	en_US
dc.type	Article	en_US