Search for Optical Variability Associated with Black Holes

Details Search for Optical Variability Associated with Black Holes Search for Optical Variability Associated with Black Holes

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1094b&link_type=abstract

HST Proposal ID #1094

Physics

Hst Proposal Id #1094

Scientific paper

It has been suggested that luminous matter passing through an accretion disk towards the event horizon of a black hole is likely to emit a short series of pulses at an increasing frequency. These so-called dying pulses trains would have a period of the order of milliseconds for stellar mass black holes. A search for such pulse trains will be made among candidate objects. Revision History: Received on RPS 9/1/89; Added to SCCS 9/5/89 RPSS V7.2 remote & local; Added data-fmt - SALM 9/7/89; Removed target NGC7078; Added target A0620-00 & related changes; Changed "contiguous exposures" to "NON-INT" - Dolan 9/26/89; Changed fluxval, ONBRD ACQ, and SAMPLE_TIME - SALM 2/14/90; Added acq to repeat sequence - SALM 6/25/90; revised time_per_exp line 0.500--BJW 7/11/90; Changed cycle 1 to cycle 2-- BJW 2/26/91; Split up proposal by cycle--BJW 3/22/91; Update target positions--BJW 7/5/91; Changed timing of observations of Cyg X-1 --BJW 9/20/91;

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