We present the first 2.05-2.45 mu m spectra of the Galactic Bulge LMXBs GX1+4 and GX13+1. We report the detection of Brackett gamma emission from the accretion disc in both systems, confirming the identification of the infrared (IR) counterpart to GX13+1. Both spectra show CO molecular bands and metal lines in absorption, representing the first IR spectroscopic detection of the secondary in a heavily obscured bulge source. We have also obtained a JHK spectrum of the LMXB Sco X-1, which shows strong H I, He I, and He II emission.
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NATL RES COUNCIL CANADA,DOMINION ASTROPHYS OBSERV,VICTORIA V8X 4M6,BC,CANADANATL RES COUNCIL CANADA,DOMINION ASTROPHYS OBSERV,VICTORIA V8X 4M6,BC,CANADA
COWLEY, AP
HUTCHINGS, JB
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NATL RES COUNCIL CANADA,DOMINION ASTROPHYS OBSERV,VICTORIA V8X 4M6,BC,CANADANATL RES COUNCIL CANADA,DOMINION ASTROPHYS OBSERV,VICTORIA V8X 4M6,BC,CANADA
HUTCHINGS, JB
CRAMPTON, D
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NATL RES COUNCIL CANADA,DOMINION ASTROPHYS OBSERV,VICTORIA V8X 4M6,BC,CANADANATL RES COUNCIL CANADA,DOMINION ASTROPHYS OBSERV,VICTORIA V8X 4M6,BC,CANADA