dc.contributor.author |
Goswami, A |
|
dc.contributor.author |
Kameswara Rao, N |
|
dc.contributor.author |
Lambert, D. L |
|
dc.date.accessioned |
2008-06-06T06:43:03Z |
|
dc.date.available |
2008-06-06T06:43:03Z |
|
dc.date.issued |
2003 |
|
dc.identifier.citation |
BASI, Vol. 31, No. 3&4, pp. 341 - 342 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2411 |
|
dc.description.abstract |
High 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.extent |
76112 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2003BASI...31..341G |
en |
dc.subject |
Star: individual |
en |
dc.subject |
Star: HD 165553 |
en |
dc.subject |
star: Variable |
en |
dc.subject |
Star: abundance |
en |
dc.title |
A Spectral Analysis of HD 165553 |
en |
dc.type |
Article |
en |