Investigation of outburst characteristics in dwarf novae binary star systems
Dwarf novae are a type of binary star system that consists of a cool red dwarf, as well as a white dwarf with an accretion disk. Occasionally the disk will get significantly brighter for a few days in an event called an outburst. On February 6th, 2002 one such system, CN Orionis, was experiencing su...
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| Format: | Others |
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2011
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| Online Access: | http://cardinalscholar.bsu.edu/handle/123456789/193590 http://liblink.bsu.edu/uhtbin/catkey/1540704 |