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A spectrophotometric study of GG Cassiopeiae

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dc.contributor.author Chaubey, U. S.
dc.contributor.author Singh, M.
dc.date.accessioned 2010-02-16T05:59:06Z
dc.date.available 2010-02-16T05:59:06Z
dc.date.issued 1989
dc.identifier.citation This article is downloaded from ADS en_US
dc.identifier.uri http://hdl.handle.net/123456789/521
dc.description.abstract The continum energy distribution of a totally eclipsing binary system GG Cas at phase 0.ᴾ903 and 0.ᴾ003 in the wavelength range λλ3200-7600 Å have been presented and discussed. The flux of continum of the secondary star seems to dominate longward of λ4500Å. The spectral types of the systemis components are found to be as B4+K0. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries ass151-335
dc.subject GG Cas en_US
dc.title A spectrophotometric study of GG Cassiopeiae en_US
dc.type Article en_US


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