dc.contributor.author |
Goswami, A |
|
dc.contributor.author |
Kameswara Rao, N |
|
dc.contributor.author |
Lambert, D. L |
|
dc.date.accessioned |
2008-09-02T15:00:24Z |
|
dc.date.available |
2008-09-02T15:00:24Z |
|
dc.date.issued |
1998-08 |
|
dc.identifier.citation |
The Observatory, Vol. 118,No. 1145, pp. 213 - 218 |
en |
dc.identifier.issn |
0029 - 7704 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3345 |
|
dc.description.abstract |
The variable star DZ Andromedae has been suspected to be an R Coronae Borealis variable. Our analysis of a high-resolution spectrum shows that the star has been misclassified: the spectrum resembles that of a K giant. We have determined the stellar parameters - effective temperature, surface gravity, and microturbulence - using model atmosphere. Abundances derived for a range of light elements, many Fe-peak elements, and a few s-process elements indicate a near-solar composition for DZ And. |
en |
dc.language.iso |
en |
en |
dc.publisher |
The Observatory |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1998Obs...118..213G |
en |
dc.subject |
Surface Gravity |
en |
dc.subject |
Micro-turbulence |
en |
dc.subject |
Stellar Parameters |
en |
dc.title |
Is DZ Andromedae an R Coronae Borealis variable? |
en |
dc.type |
Article |
en |