Investigations of Black Hole Binaries and AGN with the RXTE All Sky Monitor

Astronomy and Astrophysics – Astronomy

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Scientific paper

Results from more than one year of operation of the RXTE ASM are reviewed from the perspective of continual monitoring of both accreting binaries and active galactic nuclei. X-ray transients, including the 2 sources of superluminal radio jets, have exhibited enormously complex X-ray light curves. Progress has been achieved in our understanding the outburst mechanism via the reported detection of an optical precursor to the April 1996 outburst in GRO J1655-40. The ASM light curves have contributed to multifrequency campaigns on additional black hole binaries or candidates such as Cyg X-1, GRS1915+105, and GRS1739-278. Variations in bright extragalactic sources, such as NGC4151, Cen A, and Mkn501, are also detected, leading to new opportunities for reverberation studies made in conjunction with ground-based telescopes. The public ASM archive empowers observers with alerts for state-dependent observing opportunities. The ASM also provides a long-term context for source behavior, and this knowledge may be crucial in shaping the interpretation of brief observations with larger telescopes.

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