Identification of the Low‐Mass X‐Ray Binary and Faint X‐Ray Sources in NGC 6652
Published Version
https://doi.org/10.1086/323493Metadata
Show full item recordCitation
Heinke, 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.Abstract
We 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 sourcesTerms of Use
This article is made available under the terms and conditions applicable to Other Posted Material, as set forth at http://nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of-use#LAACitable link to this page
http://nrs.harvard.edu/urn-3:HUL.InstRepos:41399869
Collections
- FAS Scholarly Articles [17695]
Contact administrator regarding this item (to report mistakes or request changes)