X-ray emission from the cataclysmic variable PG0834+488
نویسندگان
چکیده
منابع مشابه
X-ray Variability of the Magnetic Cataclysmic Variable V1432 Aql
V1432 Aquilae (=RX J1940.2−1025) is the X-ray bright, eclipsing magnetic cataclysmic variable ∼37 away from the Seyfert galaxy, NGC 6814. Due to a 0.3% difference between the orbital (12116.3 s) and the spin (12150 s) periods, the accretion geometry changes over the ∼50 day beat period. Here we report the results of an RXTE campaign to observe the eclipse 25 times, as well as Also Universities ...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1985
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/215.1.81p