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Results from the RXTE All-Sky Monitor
Authors:Alan M Levine  Hale Bradt  Edward H Morgan  Ron Remillard  The MIT/GSFC ASM Team
Institution:

aM.I.T., Kavli Institute for Astrophysics and Space Research, Room 37-575, Cambridge, MA 02139, USA

Abstract:Selected results from the Rossi X-ray Timing Explorer All-Sky Monitor are presented to illustrate the phenomenology of the light curves. The sensitivity to periodic intensity variations is indicated by the folded light curve of AM Her. The gray line between transient and persistent sources is emphasized. Light curves of a range of systems comprising black holes or neutron stars and low and high mass companion stars show that the behavior of these systems is often, but not always, characteristic.
Keywords:X-ray binaries  Neutron stars  Black holes
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