NU Centauri: A New Beta Cephei Star

dc.contributor.author	Rajamohan, R
dc.date.accessioned	2004-11-30T11:13:04Z
dc.date.available	2004-11-30T11:13:04Z
dc.date.issued	1977
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 2, pp. 6-9	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/67
dc.description.abstract	Spectroscopic observations of the single-lined binary, NU Centauri during the years 1968-1972 were utilised to derive fresh orbital elements of this system. The measured radial velocities indicate that the primary component is a Beta Cephei type with a period of 0.1750 days	en
dc.format.extent	133810 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Spctroscopic Binaries	en
dc.subject	Variable Stars	en
dc.title	NU Centauri: A New Beta Cephei Star	en
dc.type	Article	en