Observational Evidence for the Enhancement of the Mass Transfer Rate during Dwarf Nova Outbursts

Details Observational Evidence for the Enhancement of the Mass Transfer Rate during Dwarf Nova Outbursts Observational Evidence for the Enhancement of the Mass Transfer Rate during Dwarf Nova Outbursts

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aca....45..355s&link_type=abstract

Acta Astronomica, v.45, pp.355-360, (1995).

Astronomy and Astrophysics

Astronomy

23

Novae: Cataclysmic Variables, Stars: Individual: Z Cha: U Gem

Scientific paper

Mass transfer rates in Z Cha and U Gem are determined from the
luminosity of the hot spot, taking into account the effects of the
variable radius of the disk. In both systems the mass transfer rate
increases during outburst by a factor of about2. In U Gem its subsequent
decline takes more than 40 days.

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