Far-ultraviolet fuse observations of the dwarf novae ss aurigae and ru pegasi in quiescence.
We have analyzed the Far Ultraviolet Spectroscopic Explorer (FUSE) spectra of two U Geminorum type dwarf novae, SS Aurigae and RU Pegasi, observed 28 days and 60 days (respectively) after their last outburst. In both systems, the FUSE spectra (905-1182 8) reveal evidence of the underlying accreting...
Main Authors: | , , , , |
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Format: | |
Language: | English |
Published: |
2004
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Online Access: | http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176426 |