Searching for flickering statistics in T CrB
نویسندگان
چکیده
منابع مشابه
The massive white dwarf in the recurrent nova T CrB
We have obtained I, J , H and K band light curves of the recurrent nova T CrB. We find that we can only fit the J band light curve with a Roche-lobe filling secondary star and a dark spot of radius 11–26 (90 per cent confidence) centred at the inner Lagrangian point. We obtain limits to the binary inclination of 38–46 (90 per cent confidence) which when combined with the value for the mass func...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2010
ISSN: 0035-8711,1365-2966
DOI: 10.1111/j.1365-2966.2009.16068.x