The INTEGRAL Galactic Bulge monitoring program

Details The INTEGRAL Galactic Bulge monitoring program The INTEGRAL Galactic Bulge monitoring program

2006-03-06

arxiv.org/abs/astro-ph/0603130v1

AIPConf.Proc.840:30-34,2006

Astronomy and Astrophysics

Astrophysics

5 pages, 2 figures, to be published in: "The Transient Milky Way: a perspective for MIRAX", eds. F. D'Amico, J. Braga & R. Rot

Scientific paper

10.1063/1.2216598

The Galactic Bulge region is a rich host of variable high-energy point sources. These sources include bright and relatively faint X-ray transients, X-ray bursters, persistent neutron star and black-hole candidate binaries, X-ray pulsars, etc.. We have a program to monitor the Galactic Bulge region regularly and frequently with the gamma-ray observatory INTEGRAL. As a service to the scientific community the high-energy light curves of all the active sources as well as images of the region are made available through the WWW. We show the first results of this exciting new program.

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