Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.189p..41b&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 189, Nov. 1979, p. 41P-44P.
Astronomy and Astrophysics
Astronomy
76
Dwarf Stars, Eclipsing Binary Stars, Novae, Variable Stars, Amplitudes, Light Curve, Long Term Effects, Stellar Models
Scientific paper
The cataclysmic variables UZ Boo and WX Cet both resemble WZ Sge in
showing large outburst amplitudes (approximately 8 mag), slow declines
from outbursts, and long intervals between outbursts. It is proposed
that these three stars form a distinct sub-group of the dwarf novae and
that they may all have similar binary structure.
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