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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2411
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dc.contributor.authorGoswami, A-
dc.contributor.authorKameswara Rao, N-
dc.contributor.authorLambert, D. L-
dc.date.accessioned2008-06-06T06:43:03Z-
dc.date.available2008-06-06T06:43:03Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 341 - 342en
dc.identifier.urihttp://hdl.handle.net/2248/2411-
dc.description.abstractHigh resolution spectra of HD 165553, a star reported to be a spectroscopic binary of spectral type F8 Ib are analysed. The stellar parameters - effective temperature, surface gravity and microturbulence are determined using model atmospheres. A detail chemical composition study indicates a near-solar composition for HD 165553. Comparison of its spectrum with that of Cyg, a normal supergiant of spectral type F8 Iab indicates that the star is of a later spectral type; a spectral type G Iab seems more likely for HD 165553.en
dc.format.extent76112 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..341Gen
dc.subjectStar: individualen
dc.subjectStar: HD 165553en
dc.subjectstar: Variableen
dc.subjectStar: abundanceen
dc.titleA Spectral Analysis of HD 165553en
dc.typeArticleen
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