Investigating the Sloan Digital Sky Survey Cataclysmic Variable SSDS J132723.39+652854.2
| dc.creator | Wolfe, Michael A. | |
| dc.creator | Szkody, Paula | |
| dc.creator | Fraser, Oliver J. | |
| dc.creator | Homer, Lee | |
| dc.creator | Skinner, Sam | |
| dc.creator | Silvestri, Nicole M. | |
| dc.date | 2003-05-30 | |
| dc.date | 2003-06-03 | |
| dc.date.accessioned | 2026-07-07T02:08:39Z | |
| dc.date.available | 2026-07-07T02:08:39Z | |
| dc.description | Photometric and spectroscopic observations reveal the Sloan Digital Sky Survey cataclysmic variable SDSS J132723.39+652854.2 to be a likely SW Sex star with an orbital period of P = 3.28 hours. The Sloan Digital Sky Survey spectrum shows strong HeI, HeII and Balmer emission lines. Time resolved spectra acquired at Apache Point Observatory reveal absorption-line structure within the emission lines near phase 0.5. Photometric data obtained at Manastash Ridge Observatory using Harris V and B filters reveal a high inclination system (i = 80 degrees) with deep (~ 2 mag.) eclipses. The orbital period and the spectral variations favor an SW Sex interpretation. | |
| dc.description | 12pages,7 figures. Accepted by PASP and will be published in September 2003 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0305607 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0305607 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6136 | |
| dc.subject | Astrophysics | |
| dc.title | Investigating the Sloan Digital Sky Survey Cataclysmic Variable SSDS J132723.39+652854.2 | |
| dc.type | text |