XMM-Newton observations of the low-mass X-ray binary XB1832-330 in the galactic globular cluster NGC 6652
arXiv:0805.4124 · doi:10.1051/0004-6361:200809506
Abstract
We report on two XMM-Newton observations performed in 2006 of the luminous low-mass X-ray binary XB1832-330 which is located in the galactic globular cluster NGC 6652 and is probably an ultracompact binary (orbital period less than 1 hour). The aim of these observations is to investigate the low-energy absorption towards NGC6652 and in particular to search for Ne-rich material local to the binary, which has been suggested as a possible spectral signature of Neon rich degenerate companions. XMM-Newton observed the source twice, in 2006 September and October. High resolution spectroscopy with the RGS was used to estimate the ratio of the neutral neon to oxygen column densities to search for an anomalous Ne abundance in this X-ray binary. We find no evidence for anomalous Ne/O ratios, finding Ne/O=0.18+/-0.06 and Ne/O=0.17+/-0.03 (1 sigma uncertainties), in the two observations, respectively. These values are consistent with that in the interstellar medium. Timing analysis of EPIC data suggests possible periodicities at 9170+/-235 s and 18616 +/- 531 s, which need confirmation. A by-product of these observations consists of the spatial analysis of the source field, which resulted in the detection of 46 faint sources within the EPIC field of view, which are not present in the Second XMM-Newton Serendipitous Source Catalogue. All these faint sources are likely foreground objects. We performed the first high spectral resolution observations of XB1832-33, a probable ultracompact binary, without finding any evidence for an anomalous Ne abundance.
arXiv commentAccepted for publication in A&A
References in corpus (15)
- On the Absorption of X-rays in the Interstellar Medium
- The USNO-B Catalog
- High-Resolution X-ray Spectroscopy of the Interstellar Medium: Structure at the Oxygen Absorption Edge
- Ultracompact X-Ray Binaries with Neon-Rich Degenerate Donors
- Interstellar X-ray Absorption Spectroscopy of Oxygen, Neon, and Iron with the Chandra LETGS Spectrum of X0614+091
- A highly-ionized absorber in the X-ray binary 4U 1323-62: a new explanation for the dipping phenomenon
- On the formation of neon-enriched donor stars in ultracompact X-ray binaries
- BeppoSAX study of the broad-band properties of luminous globular cluster X-ray sources
- X-Ray Spectroscopy of the Low-Mass X-ray Binaries 2S 0918-549 and 4U1543-624: Evidence for Neon-Rich Degenerate Donors
- Identification of the LMXB and Faint X-ray Sources in NGC 6652
- Looking for obscured QSOs in the X-ray emitting ERO population
- X-ray Spectroscopy of Candidate Ultracompact X-ray Binaries
- The Low-Mass X-ray Binary X1822-330 in the Globular Cluster NGC 6652: A Serendipitous ASCA Observation
- BeppoSAX study of the X-ray binary XB 1832-330 located in the globular cluster NGC 6652
- Low-energy absorption towards the ultra-compact binary 4U1850-087 located in the globular cluster NGC6712
Cited by in corpus (6)
- The gas-to-extinction ratio and the gas distribution in the Galaxy
- An Examination of the X-ray Sources in the Globular Cluster NGC 6652
- A 2.15 Hour Orbital Period for the Low Mass X-Ray Binary XB 1832-330 in the Globular Cluster NGC 6652
- The MAVERIC Survey: Variable Jet-Accretion Coupling in Luminous Accreting Neutron Stars in Galactic Globular Clusters
- XMM-Newton and INTEGRAL observations of the very faint X-ray transient IGRJ17285-2922/XTEJ1728-295 during the 2010 outburst
- The Unusual X-ray Binaries of the Globular Cluster NGC 6652