Photometric solution for the eclipsing binary TT Aurigae

dc.contributor.author	Abhyankar, K. D
dc.contributor.author	Rajasekhar Rao, N
dc.contributor.author	Lokanadham, B
dc.date.accessioned	2005-02-09T06:17:25Z
dc.date.available	2005-02-09T06:17:25Z
dc.date.issued	1982-12
dc.identifier.citation	BASI, Vol. 10, No. 4, pp. 323-328	en
dc.identifier.uri	http://hdl.handle.net/2248/350
dc.description.abstract	Photometric elements of TT Aur are derived from the UBV observations of the star during 1973-77. The system is found to be detached but quite close. Absolute dimensions are obtained on the basis of the spectroscopic element given by Joy & Sitterly (1931). It appears that the radial velocity amplitudes found by them might need upward revision by about 50 km/s.	en
dc.format.extent	421709 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	TT Aur	en
dc.subject	eclipsing binary	en
dc.subject	photometry	en
dc.title	Photometric solution for the eclipsing binary TT Aurigae	en
dc.type	Article	en