XMM-Newton observations of the low-mass X-ray binary XB 1832–330 in the galactic globular cluster NGC 6652

2008/05/27 by L. Sidoli, N. La Palombara, T. Oosterbroek +1
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Binary number #Binary star #Binary system #Cluster (spacecraft) #Globular cluster #Open cluster #Star cluster #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809506

Accepted for publication in A&A

arxiv created 2008/05/27 · openalex publication_date 2008/07/09 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. We report on two XMM-Newton observations performed in 2006 of the luminous low-mass X-ray binary XB 1832–330, which is located in the galactic globular cluster NGC 6652 and is probably an ultracompact binary (orbital period, Porb, of <1 h).

Citations

• Identification of the Low‐Mass X‐Ray Binary and Faint X‐Ray Sources in NGC 6652
• X‐Ray Spectroscopy of Candidate Ultracompact X‐Ray Binaries
• X‐Ray Spectroscopy of the Low‐Mass X‐Ray Binaries 2S 0918−549 and 4U 1543−624: Evidence for Neon‐rich Degenerate Donors
• A Catalog of Parameters for Globular Clusters in the Milky Way
• BeppoSAX study of the X-ray binary XB1832-330 located in the globular cluster NGC6652
• The USNO-B Catalog