dc.contributor.author |
Kameswara Rao, N |
|
dc.contributor.author |
Lambert, D. L |
|
dc.date.accessioned |
2008-09-17T11:37:40Z |
|
dc.date.available |
2008-09-17T11:37:40Z |
|
dc.date.issued |
2003-11 |
|
dc.identifier.citation |
The Publications of the Astronomical Society of the Pacific, Vol. 115, No. 813, pp. 1304 - 1307 |
en |
dc.identifier.issn |
0004 - 6280 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3698 |
|
dc.description.abstract |
Photometry and low-resolution spectroscopy have added V2552 Oph to the rare class of R Coronae Borealis variables. We confirm this classification of V2552 Oph through a comparison of our high-resolution optical spectrum of this star and that of R CrB and other F-type members of the class. We show that V2552 Oph most closely resembles Y Mus and FH Sct, stars in which Sr, Y, and Zr are enhanced. |
en |
dc.language.iso |
en |
en |
dc.publisher |
The Astronomical Society of the Pacific |
en |
dc.relation.uri |
http://dx.doi.org/10.1086/379205 |
en |
dc.subject |
Stars:Individual (V2552 Ophiuchi) |
en |
dc.subject |
Photometry |
en |
dc.title |
A High-Resolution Spectrum of the R Coronae Borealis Star V2552 Ophiuchi |
en |
dc.type |
Article |
en |