| 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 |