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NTIS 바로가기천문학논총 = Publications of the Korean Astronomical Society, v.30 no.2, 2015년, pp.237 - 240
SURINA, FARUNG (Department of Science and Technology, Chiangrai Rajabhat University) , BODE, MICHAEL F. (Astrophysics Research Institute, Liverpool John Moores University) , DARNLEY, MATTHEW J. (Astrophysics Research Institute, Liverpool John Moores University)
Classical novae (CNe) are interacting binary systems whose outbursts are powered by a thermonuclear runaway in accreted material onto the surface of a white dwarf (WD). The secondary star in such systems fills its Roche lobe and material is transferred onto the WD primary star via an accretion disk....
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