The 0.33 Day DA Plus dMe Binary BPM 6502
| dc.contributor.author | Kawka, Adela | |
| dc.contributor.author | Vennes, Stephane | |
| dc.contributor.author | Dupuis, Jean | |
| dc.contributor.author | Koch, Rolf | |
| dc.date.accessioned | 2015-12-13T23:18:24Z | |
| dc.date.available | 2015-12-13T23:18:24Z | |
| dc.date.issued | 2000 | |
| dc.date.updated | 2015-12-12T08:56:37Z | |
| dc.description.abstract | We have obtained a series of spectroscopic measurements of the high proper-motion star BPM 6502 showing Balmer emission superposed upon the absorption lines. Radial velocity measurements determined by tracing optical absorption and emission lines show that the star is a binary system comprised of a DA white dwarf and an M dwarf with an orbital period of 0.33678 days. The space motion of the system falls within the general white dwarf population, and the system is not expected to initiate mass transfer within a Hubble time. | |
| dc.identifier.issn | 0004-6256 | |
| dc.identifier.uri | http://hdl.handle.net/1885/90155 | |
| dc.publisher | University of Chicago Press | |
| dc.source | Astronomical Journal | |
| dc.subject | Keywords: Binaries: close; Stars: individual (BPM 6502); Ultraviolet emission; White dwarfs | |
| dc.title | The 0.33 Day DA Plus dMe Binary BPM 6502 | |
| dc.type | Journal article | |
| local.bibliographicCitation.issue | 6 | |
| local.bibliographicCitation.lastpage | 3254 | |
| local.bibliographicCitation.startpage | 3250 | |
| local.contributor.affiliation | Kawka, Adela, University of Durham | |
| local.contributor.affiliation | Vennes, Stephane, College of Physical and Mathematical Sciences, ANU | |
| local.contributor.affiliation | Dupuis, Jean, University of California | |
| local.contributor.affiliation | Koch, Rolf, Murdoch University | |
| local.contributor.authoruid | Vennes, Stephane, u9711096 | |
| local.description.notes | Imported from ARIES | |
| local.description.refereed | Yes | |
| local.identifier.absfor | 020110 - Stellar Astronomy and Planetary Systems | |
| local.identifier.ariespublication | MigratedxPub20443 | |
| local.identifier.citationvolume | 120 | |
| local.identifier.scopusID | 2-s2.0-0038584801 | |
| local.type.status | Published Version |