Continued M31 Monitoring for Black Hole X-ray Nova

Details Continued M31 Monitoring for Black Hole X-ray Nova Continued M31 Monitoring for Black Hole X-ray Nova

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006hst..prop11013g&link_type=abstract

HST Proposal ID #11013. Cycle 15

Physics

Scientific paper

We have been carring out a Chandra GO+GTO and HST GO program to find Black Hole X-ray Nova BHXN and their optical counterparts in M31 for several years. To date we have found >2 dozen BHXN and 3 HST optical counterparts for these BHXN. Our results suggest a rather high ratio of BH to neutron star NS binaries, or a high duty cycle for the BHXN. We propose to continue this program, with the goal of determining the orbital period distribution and duty cycles of these BHXN. Current results yield 3 orbital periods and 3 upper limits. Our proposed observations will ~double the total number of periods and therefore yield sufficient numbers to make a first approximation of the orbital period distribution. The orbital period distribution is the fundamental observable parameter any binary stellar evolution models must match, and the duty cycle is very poorly known but directly influences the binary lifetime. M31 is the only galaxy in which this extra-galactic study of BHXN is feasible. Furthermore, the 2 HST observations will allow us to estimate the orbital period of a single super-Eddington source.

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