Relativistic Effects and Outflows in a Black Hole Transient

Details Relativistic Effects and Outflows in a Black Hole Transient Relativistic Effects and Outflows in a Black Hole Transient

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1670m&link_type=abstract

Chandra Proposal ID #06400177

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Chandra Proposal Id #06400177

Scientific paper

Our Chandra observations of Galactic BH systems have begun to reveal relativistic effects and important connections between stellar-mass black holes and the super-massive black holes powering Seyferts, including relativistic iron emission lines and outflowing warm absorber geometries. We propose to observe a Galactic BH transient in outburst for 200 ksec, in 4 obs. of 50 ksec, using the HETGS. These observations will probe relativistic effects near black holes, the nature and evolution of disk winds and warm absorbers, the emerging disk-jet connection in BH systems, and the dependence of the accretion flow geometry on mass accretion rate and other parameters. These observations will be supported by a global multi-wavelength (radio, IR, optical, X-ray, gamma-ray) program.

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