Recent progress in understanding QPO sources

Details Recent progress in understanding QPO sources Recent progress in understanding QPO sources

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987txra.symp..504b&link_type=abstract

13th Texas Symposium on Relativistic Astrophysics, p. 504 - 508

Astronomy and Astrophysics

Astrophysics

1

Neutron Stars, Stellar Luminosity, Stellar Mass Accretion, Stellar Models, Stellar Oscillations, X Ray Stars, Coherent Electromagnetic Radiation, Compton Effect, Cygnus Constellation, Stellar Coronas, Stellar Rotation

Scientific paper

New observational and theoretical results strongly suggest that QPOs in the fast, luminous sources are caused by oscillations in the luminosity of the X-ray star. They also explain why coherent pulsations at the stellar rotation frequency are so weak in these sources. Observations of weak red noise suggest that the luminosity oscillations in some sources are partially coherent.

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