A phenomenological analysis of the spectral bimodality in the QPO object GX5 - 1

Details A phenomenological analysis of the spectral bimodality in the QPO object GX5 - 1 A phenomenological analysis of the spectral bimodality in the QPO object GX5 - 1

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acaps..10..299y&link_type=abstract

(Acta Astrophysica Sinica, vol. 10, no. 4, 1990, p. 299-305) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15, March

Astronomy and Astrophysics

Astrophysics

Neutron Stars, Stellar Mass Accretion, Stellar Oscillations, X Ray Binaries, Spectrum Analysis, Stellar Rotation, X Ray Sources

Scientific paper

Some corrections and improvements to the beat frequency model for the quasi-periodic oscillation phenomenon in X-ray binaries are made in this paper. The main point is that viscous damping in the column accretion process has been included in the consideration and this has led to a successful explanation of the two-branch spectrum, unaccounted for by the previous beat frequency model.

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