Physics
Scientific paper
Feb 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010noao.prop..399r&link_type=abstract
NOAO Proposal ID #2010A-0399
Physics
Scientific paper
Probing General Relativity in the strong field regime and understanding the production of relativistic jets are two critical issues in the study of X-ray binaries. In both of these areas the Galactic microquasar GRS 1915+105 occupies a unique place in our effort to address these questions: in addition, it is nominally the most massive of all known stellar-mass Galactic black holes. However, a reanalysis of archival VLT data shows that this mass estimate is likely subject to significant systematic uncertainty. We propose new observations, which should lead to a more reliable mass estimate for the black hole in this system.
Callanan Paul
Hurley Dan
Miller Jon
Reynolds Mark
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