The possibility of hydrogen-like and helium-like iron K? line emission from the black hole X-ray binary

Details The possibility of hydrogen-like and helium-like iron K? line emission from the black hole X-ray binary The possibility of hydrogen-like and helium-like iron K? line emission from the black hole X-ray binary

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002acasn..43..284x&link_type=abstract

Acta Astronomica Sinica, vol.43, no.3, p. 284-292

Physics

Accretion, Accretion Disk, Black Hole Physics, Star: Individual: Gx339-4, X -Rays: Binaries, Methods: Analytical

Scientific paper

The iron K? line emission from the black hole X-ray binary GX339-4 in the `off' state is calculated. It is shown that the black hole which accretes via ADAF (advection-dominated accretion flow) with very low accretion rate might produce detectable H-like and He-like iron K? lines of sufficient strength . Although ADAF model has been applied successfully in explaining the continuum spectra of many low accretion rate systems. The line emission from ADAF has rarely been discussed till now.

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