Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...396l..27m&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 396, no. 1, Sept. 1, 1992, p. L27-L30. Research supported by Alfr
Astronomy and Astrophysics
Astrophysics
3
Accretion Disks, Binary Stars, Hydrodynamic Equations, Neutron Stars, Radiative Transfer, Stellar Coronas, Astronomical Models, Globular Clusters, Light Curve, X Ray Binaries, X Ray Scattering
Scientific paper
A fully self-consistent radiative hydrodynamical algorithm developed earlier is used to study the 'steady' state coronae in order to simulate the response of the evaporated outflow to a time-dependent irradiation of the disk's surface. It is found that the burst definition is altered at both low and high inclination angles i. At i greater than or approximately equal to 45 deg, the detectable flux is enhanced (as much as 50 percent) by X-rays scattered into the line of sight from the radiation propagation through the corona, and (greater than or approximately equal to 30 percent) by X-rays reflected off the corona when i is less than or approximately equal to 45 deg.
Fryxell Bruce
Melia Fulvio
Zylstra Gregory J.
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