The luminosity oscillation of X-ray bursters and recurrent novae

Details The luminosity oscillation of X-ray bursters and recurrent novae The luminosity oscillation of X-ray bursters and recurrent novae

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.138...41a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 138, no. 1, Nov. 1987, p. 41-48.

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Gamma Ray Bursts, Globular Clusters, Novae, Stellar Luminosity, Stellar Oscillations, X Ray Sources, Binary Stars, Computational Astrophysics, Giant Stars, Stellar Atmospheres, Upper Atmosphere, White Dwarf Stars

Scientific paper

`Thermo-mechanical' oscillations of a radiating spherically-symmetric shell containing a fermion gas (i.e., oscillation where only mechanical, thermodynamical, and eventually radiation phenomena are taken into account) are studied. With a reasonable choice of the three relevant parameters all other observational data are similar to the ones of X-ray bursters and recurrent novae. Therefore, thermo-mechanical oscillations could play an important role in the oscillation spectrum of these astronomical objects.

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