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X-Ray Binaries

  • Thierry J.-L. Courvoisier
Chapter
Part of the Astronomy and Astrophysics Library book series (AAL)

Abstract

The very different nature of the emission mechanisms at the origins of X-ray and visible emission makes it inevitable that the sky looks very different in these two wavebands. This is illustrated by Fig. 16.1 which shows the bulge of our Galaxy observed in the hard X-rays by INTEGRAL (top), and in the visible domain (bottom). This illustrates how essential multi-wavelength observations are. One simply cannot discover or understand objects that emit the bulk of their luminosity in the X-rays from optical observations alone. The same line of argument holds for all wavebands.

Keywords

Black Hole Neutron Star Accretion Disk Accretion Rate Compact Object 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2013

Authors and Affiliations

  • Thierry J.-L. Courvoisier
    • 1
  1. 1.ISDC, Data Centre for Astrophysics University of GenevaVersoixSwitzerland

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