SIMBAD references

2012ApJ...757..169C - Astrophys. J., 757, 169 (2012/October-1)

The X-ray transient 2XMMi J003833.3+402133: a candidate magnetar at high galactic latitude.

CALLINGHAM J.R., FARRELL S.A., GAENSLER B.M., LEWIS G.F. and MIDDLETON M.J.

Abstract (from CDS):

We present detailed analysis of the transient X-ray source 2XMMi J003833.3+402133 detected by XMM-Newton in 2008 January during a survey of M31. The X-ray spectrum is well fitted by either a steep power law plus a blackbody model or a double blackbody model. Prior observations with XMM-Newton, Chandra, Swift, and ROSAT spanning 1991-2007, as well as an additional Swift observation in 2011, all failed to detect this source. No counterpart was detected in deep optical imaging with the Canada-France-Hawaii Telescope down to a 3σ lower limit of g = 26.5 mag. This source has previously been identified as a black hole X-ray binary in M31. While this remains a possibility, the transient behavior, X-ray spectrum, and lack of an optical counterpart are equally consistent with a magnetar interpretation for 2XMMi J003833.3+402133. The derived luminosity and blackbody emitting radius at the distance of M31 argue against an extragalactic location, implying that if it is indeed a magnetar it is located within the Milky Way but 22° out of the plane. The high Galactic latitude could be explained if 2XMMi J003833.3+402133 were an old magnetar, or if its progenitor was a runaway star that traveled away from the plane prior to going supernova.

Abstract Copyright:

Journal keyword(s): galaxies: individual: M31 - stars: neutron - X-rays: individual: 2XMMi J003833.3+402133 - X-rays: stars

Simbad objects: 11

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2012ApJ...757..169C and select 'bookmark this link' or equivalent in the popup menu


2021.06.19-08:03:14

© Université de Strasbourg/CNRS

    • Contact