Keck K-band observations of low mass X-ray binaries

Details Keck K-band observations of low mass X-ray binaries Keck K-band observations of low mass X-ray binaries

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..599..433c&link_type=abstract

X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. Edited by Nicholas E. White, Giuseppe Malaguti, and G

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1

X-Ray Binaries, Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Cataclysmic Binaries, Symbiotic Stars

Scientific paper

We present K-band observations of a sample of XRN/LMXB using NIRC on
Keck I. For GRO J0422+32, we show that the K-band flux is significantly
contaminated by the accretion disk. We present K-band images of 4U
1630-47, Aql X-1, and GX 17+2, and we discuss the implications of the
newly discovered IR/optical counterparts for the latter two systems. .

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