Time-dependent models of Soft X-ray Transients

Details Time-dependent models of Soft X-ray Transients Time-dependent models of Soft X-ray Transients

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.349m&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We develop time-dependent numerical models of accretion flows in Soft X-ray Transients. We assume that accretion in these systems occurs via an outer thin accretion disk and an inner advection-dominated accretion flow (ADAF).The two components of the accretion flow are combined self-consistently: accretion via the ADAF results from evaporation of the thin disk in quiescence and the influence of the soft emission from the disk is taken into account in the radiative calculations for the ADAF.

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