Document Type
Article
Publication Date
2-1-1995
Publication Title
Monthly Notices of the Royal Astronomical Society
Department
Department of Physics and Astronomy
Abstract
Several pre-cataclysmic binaries, comprising a hot white dwarf with a red dwarf companion, have been discovered as a result of the optical identification of EUV sources from the ROSAT all-sky survey. The optical spectra have the steep blue continuum and Balmer absorption typical of a hot white dwarf, but there are bright, narrow emission lines of H I (and sometimes He I and Ca II) superimposed. An intense campaign of follow-up observations has been devoted to these binary systems. So far, only RE 2013+400 has exhibited any measurable changes in the radial velocities of the emission components, from which it is possible to estimate that the binary period is 0.71 d. A clear He II 4886-Å absorption feature is detected, which indicates that, like most PCBs with white dwarfs hotter than 40 000 K, the white dwarf is a hydrogen-helium hybrid star (DAO). A combined analysis of the optical, UV and EUV/X-ray data suggests that the atmospheric He abundance is higher in the optical line-forming region of the white dwarf photosphere than in the region where the EUV/X-ray flux is formed. This is an interesting result, in the light of the recent optical study of a sample of DAO white dwarfs by Bergeron et al., if representative of DAO white dwarfs in general.
DOI
10.1093/mnras/272.3.531
Dartmouth Digital Commons Citation
Barstow, M. A.; Burleigh, M. R.; Fleming, T. A.; Holberg, J. B.; Koester, D.; Marsh, M. C.; Rosen, S. R.; Rutten, R. G.M.; Sakai, S.; Tweedy, R. W.; and Wegner, G., "The Orbital Period of the Pre-Cataclysmic Binary RE 2013+400 and a Study of the Atmosphere of the DAO White Dwarf Primary" (1995). Dartmouth Scholarship. 3437.
https://digitalcommons.dartmouth.edu/facoa/3437
