Interpretation of the light curves of ``quiescent'' X-ray novae in a model with a noncollisional interaction between the flow and disk. The XTE J1118+480 system

Details Interpretation of the light curves of ``quiescent'' X-ray novae in a model with a noncollisional interaction between the flow and disk. The XTE J1118+480 system Interpretation of the light curves of ``quiescent'' X-ray novae in a model with a noncollisional interaction between the flow and disk. The XTE J1118+480 system

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005arep...49...79k&link_type=abstract

Astronomy Reports, vol. 49, Issue 2, p.79-88

Astronomy and Astrophysics

Astronomy

3

Scientific paper

We have analyzed the orbital light curve of the X-ray nova XTE J1118+480 in a “disk + hot line” model based on three-dimensional gas-dynamical computations of gas flows in interacting binary systems. As a result, we have been able to derive reliable parameters for the system: i = 80 -4 +4 degrees, MBH = 7.1 -0.1 +0.5 M &sun;, M opt = 0.39 -0.07 +0.15 M &sun;.

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