Modelling the extreme ultraviolet emission during the low state of Hercules X-1

Details Modelling the extreme ultraviolet emission during the low state of Hercules X-1 Modelling the extreme ultraviolet emission during the low state of Hercules X-1

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mnras.342..446l&link_type=abstract

Monthly Notice of the Royal Astronomical Society, Volume 342, Issue 2, pp. 446-452.

Astronomy and Astrophysics

Astronomy

4

Binaries: Eclipsing, Stars: Individual: Hz Her/Her X-1, Stars: Neutron

Scientific paper

Hercules X-1 was observed for extended periods during its low state by the Extreme Ultraviolet Explorer (EUVE). These observations yield low-state light curves in the extreme ultraviolet (EUV) which are compared with a composite model here. The model includes reflection of soft X-rays off the companion HZ Her, including the shadowing of HZ Her by the accretion disc, and emission from the accretion disc surface. Four different geometries for the accretion disc were adopted, all derived from the RXTE All-Sky Monitor (ASM) 35-day light-curve modelling. Three were thin disc models for different system inclinations, i, and the fourth was a disc with a thick inner ring for i= 85°.
With the HZ Her reflection model, with no free parameters except normalization, and a simple model for the disc emission, the models fit the data well. The disc emission accounts for about half of the EUV flux, depending on which accretion disc geometry is used. The disc geometry that best fits the EUV light curves is the disc with a thick inner ring, which is the same model that gives the best fit to the RXTE/ASM light curve.

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