Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/350
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dc.contributor.authorAbhyankar, K. D-
dc.contributor.authorRajasekhar Rao, N-
dc.contributor.authorLokanadham, B-
dc.date.accessioned2005-02-09T06:17:25Z-
dc.date.available2005-02-09T06:17:25Z-
dc.date.issued1982-12-
dc.identifier.citationBASI, Vol. 10, No. 4, pp. 323-328en
dc.identifier.urihttp://hdl.handle.net/2248/350-
dc.description.abstractPhotometric 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.extent421709 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectTT Auren
dc.subjecteclipsing binaryen
dc.subjectphotometryen
dc.titlePhotometric solution for the eclipsing binary TT Aurigaeen
dc.typeArticleen
Appears in Collections:BASI Publications

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