Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-02T20:45:37.562Z Has data issue: false hasContentIssue false
  • English
  • Français

Chandra Multi-wavelength Plane Survey

Published online by Cambridge University Press:  21 February 2013

Ping Zhao ,
Jonathan E. Grindlay ,
Jaesub Hong ,
Mathieu Servillat  and
Maureen van den Berg
Ping Zhao
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
Jonathan E. Grindlay
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
Jaesub Hong
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
Mathieu Servillat
Affiliation:
CEA Scalay, France
Maureen van den Berg
Affiliation:
University of Amsterdam, The Netherlands
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Chandra Multi-wavelength Plane Survey (ChaMPlane) surveys the X-ray point sources discovered by the Chandra X-ray Observatory in the galactic plane in order to constrain the populations of faint (Lx ≤ 1033erg/s) accretion-powered sources in the Galaxy. This multi-wavelength survey includes data from the Chandra archive, as well as optical and infrared images and spectra. This paper summarizes a few selected highlights.

Keywords

Chandra X-ray ObservatorySurveyGalactic planeAccretionX-ray binariesCVs
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 157 - 160
Copyright
Copyright © International Astronomical Union 2013

References

Grindlay, J. E.et al. 2003, Astronomische Nachrichten, V324, No.1–2, 57–60Google Scholar
Grindlay, J. E.et al. 2005, ApJ, 635, 920CrossRefGoogle Scholar
Drimmel, & Spergel, 2001, ApJ, 556, 181Google Scholar
Hong, J.et al. 2004, ApJ, 614, 508CrossRefGoogle Scholar
Hong, J.et al. 2005, ApJ, 635, 907Google Scholar
Hong, J.et al. 2009, ApJ, 706, 223Google Scholar
Koenig, X.et al. 2008, ApJ, 685, 463CrossRefGoogle Scholar
Wang, D.et al. 2002, Nature, 415, 148Google Scholar
Zhao, P.et al. 2003, Astronomische Nachrichten, V324, No.1–2, 176Google Scholar
Zhao, P.et al. 2005, ApJS, 161, 429CrossRefGoogle Scholar