Photometric Observations of Eccentric Accretion in Algol-type Binary Stars
Some Algol-type interacting binary stars exhibit strange photometric variations that can be phase-dependent and/or secular. This paper discusses the possibility of explaining these observed variations as resulting from an accretion structure eclipsing one or both of the stars. Some previous studies...
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Format: | Article |
Language: | English |
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Korean Space Science Society (KSSS)
2012-06-01
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Series: | Journal of Astronomy and Space Sciences |
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Online Access: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2012/v29n2/OJOOBS_2012_v29n2_141.pdf |