QZ Aurigae: An eclipsing cataclysmic variable with a white dwarf of almost equivalent mass to its companion | Zendy

Guang Shi | Zendy; S. Qian | Zendy

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QZ Aurigae: An eclipsing cataclysmic variable with a white dwarf of almost equivalent mass to its companion

Author(s) -

Guang Shi,

S. Qian

Publication year - 2014

Publication title -

publications of the astronomical society of japan

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.99

H-Index - 110

eISSN - 2053-051X

pISSN - 0004-6264

DOI - 10.1093/pasj/psu004

Subject(s) - physics , white dwarf , astrophysics , orbital period , eclipse , cataclysmic variable star , astronomy , light curve , observatory , dwarf nova , intermediate polar , telescope , mass ratio , binary star , stars

We present CCD photometric monitoring of the classic nova QZ Aurigae (Nova Aur 1964) since 2008 with the 2.4-m telescope at Lijiang station of Yunnan Astronomical Observatory in China, as well as the 2.16-m telescope and the 85-cm telescope at Xionglong station of the National Astronomical Observatory in China. By utilizing eight new eclipse timings and the data from the last literature, published...

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