Time-resolved spectroscopy of the AM Herculis-type binary systems QQ VUL and EF ERI
Cataclysmic variable stars (CVs) are interacting binary systems. One of the stars (referred to as the primary) is a white dwarf, the other (referred to as the secondary) is usually a late main sequence star such as a red dwarf. Due to the closeness of the two stars, the white dwarf accretes gasses f...
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| Format: | Others |
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2011
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| Online Access: | http://cardinalscholar.bsu.edu/handle/handle/186131 http://liblink.bsu.edu/uhtbin/catkey/1115429 |