Variable Broadband SEDs for Neutron Star Low-Mass X-ray Binaries

Details Variable Broadband SEDs for Neutron Star Low-Mass X-ray Binaries Variable Broadband SEDs for Neutron Star Low-Mass X-ray Binaries

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.1011c&link_type=abstract

American Astronomical Society, HEAD meeting #10, #10.11

Astronomy and Astrophysics

Astronomy

Scientific paper

We present broadband spectral energy distributions (SEDs) from radio through to X-rays for 6 neutron star low-mass X-ray binaries. Each object was observed at 2 separate epochs with simultaneous observations in each band allowing for a study of the variable components in the SED and how they are correlated across the wavebands. We compare the broadband properties and changes with the location of the source on the X-ray color-color diagram and with absorption and emission line properties in the Chandra HETGS spectra. In addition, we study the relative contribution of the jet and reprocessing at IR and optical wavelengths and compare this to what has been observed in black hole LMXBs at similar fractions of Eddington.

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