Probe the relativistic Out-flow in the microquasar GRS1915+105 with HETG/Chandra

Details Probe the relativistic Out-flow in the microquasar GRS1915+105 with HETG/Chandra Probe the relativistic Out-flow in the microquasar GRS1915+105 with HETG/Chandra

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cxo..prop.1439f&link_type=abstract

Chandra Proposal ID #05400884

Physics

Chandra Proposal Id #05400884

Scientific paper

In the microquasar GRS 1915+105, radio and X-ray flares have been found to be correlated in some episodes. The radio jet forms during the plateau flare. In 1998 during a radio/X-ray flare, the blue shifted absorption lines were observed with ASCA, which indicates a strong jet/out-flow, which enables us to probe the velocity and density distribution of the jet/out-flow. We propose to monitor the microquasar GRS 1915+105 with ACIS-S/HETG. The observation will provide the first detailed X-ray spectroscopy data on GRS 1915+105 during a correlated radio/X-ray flare and also allow us to study the correlation between the properties of the the jet and those of the accretion disk.

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