DZ Andromedae : A search for the spectral evidence of its possible RCB nature

dc.contributor.author	Goswami, A
dc.contributor.author	Kameswara Rao, N
dc.contributor.author	Lambert, D. L
dc.date.accessioned	2007-10-19T09:13:47Z
dc.date.available	2007-10-19T09:13:47Z
dc.date.issued	1999
dc.identifier.citation	BASI, Vol. 27, No. 1, pp. 129 - 132	en
dc.identifier.uri	http://hdl.handle.net/2248/1908
dc.description.abstract	The analysis of high-resolution spectra of DZ Andromedae, a suspected R Coronae Borealis variable, is presented here. The spectra of DZ And show the characteristics of a normal K2 III star, indicating that the star was earlier misclassifed. A detailed abundance analysis also indicates that the star's composition is not consistent with its membership in the RCB class.	en
dc.format.extent	214190 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1999BASI...27..129G	en
dc.subject	DZ Andromedae	en
dc.subject	RCB stars	en
dc.title	DZ Andromedae : A search for the spectral evidence of its possible RCB nature	en
dc.type	Article	en