The detection of an X-ray outburst from the old nova GK Per

Details The detection of an X-ray outburst from the old nova GK Per The detection of an X-ray outburst from the old nova GK Per

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.187p..77k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 187, June 1979, p. 77P-81P.

Astronomy and Astrophysics

Astronomy

22

Light Curve, Novae, Stellar Mass Accretion, White Dwarf Stars, X Ray Sources, Radial Flow, Radiation Detectors, Secondary Flow, Stellar Models

Scientific paper

The detection of an X-ray outburst from the old nova GK Per at a time
when the object had brightened optically by about 1 mag is reported. The
outburst is interpreted in terms of an increased rate of accretion of
material from the secondary via Roche-lobe overflow onto the white dwarf
of the system.

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