Summarizing ChaMPlane: Global Distributions And Nature Of Faint Chandra XRBs in the Galaxy

Details Summarizing ChaMPlane: Global Distributions And Nature Of Faint Chandra XRBs in the Galaxy Summarizing ChaMPlane: Global Distributions And Nature Of Faint Chandra XRBs in the Galaxy

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011head...12.1305g&link_type=abstract

American Astronomical Society, HEAD meeting #12, #13.05

Astronomy and Astrophysics

Astronomy

Scientific paper

We summarize the global properties of sources detected in our nearly 10y ChaMPlane survey of faint (<0.01 cts/s) Chandra sources in the Galactic plane. In this presentation, we focus on sources detected above 2 keV which are dominated by CVs and XRBs. Using the GCR hard sources with optical counterparts (Zhao et al), we derive constraints on luminosity and spatial distributions for sources out to 3 kpc (for NH < 3 E21) for comparison with all ChaMPlane fields with similar limiting NH to constrain the global distributions of CVs and qLMXBs in the Galaxy.

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