Spitzer Observations of Low Mass X-ray Binaries

Details Spitzer Observations of Low Mass X-ray Binaries Spitzer Observations of Low Mass X-ray Binaries

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.1031w&link_type=abstract

American Astronomical Society, HEAD meeting #10, #10.31

Astronomy and Astrophysics

Astronomy

Scientific paper

We present results from our archival Spitzer Space Telescope program aimed at characterizing the mid-IR properties of compact objects, both isolated and in binary systems, i.e. white dwarfs, X-ray binaries, cataclysmic variables, and magnetars. Most of these sources are too faint at mid-IR wavelengths to be observable from the ground, so this study provides the very first comprehensive look at the mid-IR emission of these objects. Here we present our results for the low mass X-ray binaries. We considered all of the systems listed in the most recent catalog of Liu et al. 2007 that have known optical counterparts. The particular goals of our projects encompass: to establish the mid-IR spectral energy distribution, to search for the signatures of jets, circumbinary disks, low mass or planetary companions and debris disks, and to study the local environment of these sources.

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