Deriving an X-ray luminosity function of dwarf novae

Details Deriving an X-ray luminosity function of dwarf novae Deriving an X-ray luminosity function of dwarf novae

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..145b&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

Dwarf Novae, X-Ray Sources (Astronomical), Brightness, Astronomical Telescopes, Galaxies, Cataclysmic Binaries, Symbiotic Stars, X-Ray Sources, X-Ray Bursts, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, X- And Gamma-Ray Telescopes And Instrumentation, Galaxy Clusters

Scientific paper

Current measurements of X-ray luminosity functions of dwarf novae contain biases due to high X-ray flux sources. We have obtained Suzaku, XMM-Newton and ASCA observations of nearby DNe which have parallax-based distance measurements, and carried out X-ray spectral analysis for these sources. Our primary goal is to derive a reliable X-ray luminosity function for this sample, and to compare it with existing X-ray luminosity functions. We briefly introduce the source sample and preliminary results.

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