Solar cycle model for oscillating transient X-ray sources

Details Solar cycle model for oscillating transient X-ray sources Solar cycle model for oscillating transient X-ray sources

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..42..165a&link_type=abstract

(COSPAR, Symposium on Fast Transients in X- and Gamma-Rays, Varna, Bulgaria, May 29-31, 1975.) Astrophysics and Space Science, v

Astronomy and Astrophysics

Astrophysics

Binary Stars, Solar Cycles, Stellar Rotation, White Dwarf Stars, X Ray Sources, Ariel Satellites, Astronomical Models, Neutron Stars, Stellar Envelopes, Stellar Magnetic Fields, Stellar Models

Scientific paper

The oscillations observed recently in the transient X-ray source
A1118-61 are attributed to variations in the magnetic activity of a
rotating white dwarf similar to the 11-year solar activity cycle. The
transient nature, in analogy with the sun, is attributed to the
variation in the strength of the cycle.

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