Identification of the Low‐Mass X‐Ray Binary and Faint X‐Ray Sources in NGC 6652
Heinke, C. O.
Edmonds, P. D.
Grindlay, J. E.
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CitationHeinke, C. O., P. D. Edmonds, and J. E. Grindlay. 2001. “Identification of the Low‐Mass X‐Ray Binary and Faint X‐Ray Sources in NGC 6652.” The Astrophysical Journal 562 (1): 363–67. https://doi.org/10.1086/323493.
AbstractWe have detected three new X-ray point sources, in addition to the known low-mass X-ray binary (LMXB) X1832-330, in the globular cluster NGC 6652 with a Chandra 1.6 ks HRC-I exposure. Star 49 (M-V similar to 4.7), suggested by Deutsch and coworkers as the optical candidate for the LMXB, is identified (<0.<double prime>3) not with the LMXB, but with another, newly detected source (B). Using archival Hubble Space Telescope (HST) images, we identify (<0.<double prime>3) the LMXB (A) and one of the remaining new sources
Citable link to this pagehttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41399869
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