Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-05-27
Astronomy and Astrophysics
Astrophysics
Scientific paper
10.1086/591494
We present an analysis of the Far Ultraviolet Spectroscopic Explorer ({\it{FUSE}}) spectra of the little-known southern nova-like BB Doradus. The spectrum was obtained as part of our Cycle 8 {\it FUSE} survey of high declination nova-like stars. The FUSE spectrum of BB Dor, observed in a high state, is modeled with an accretion disk with a very low inclination (possibly lower than 10deg). Assuming an average WD mass of 0.8 solar leads to a mass accretion rate of 1.E-9 Solar mass/year and a distance of the order of 650 pc, consistent with the extremely low galactic reddening in its direction. The spectrum presents some broad and deep silicon and sulfur absorption lines, indicating that these elements are over-abundant by 3 and 20 times solar, respectively.
Barrett Paul Everett
Godon Patrice
Schlegel Eric M.
Sion Edward M.
Szkody Paula
No associations
LandOfFree
Far Ultraviolet Spectroscopic Explorer Spectroscopy of the Nova-like BB Doradus does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Far Ultraviolet Spectroscopic Explorer Spectroscopy of the Nova-like BB Doradus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Far Ultraviolet Spectroscopic Explorer Spectroscopy of the Nova-like BB Doradus will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-415595