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XMM-Newton reveals ∼100 new LMXBs in M31 from variability studies

Barnard, R.; Shaw Greening, L.; Tonkin, C.; Kolb, U. and Osborne, J. P. (2006). XMM-Newton reveals ∼100 new LMXBs in M31 from variability studies. In: Populations of high energy sources in galaxies: proceedings of the 230th symposium of the International Astronomical Union, 15-19 August 2005, Dublin, Ireland.

DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1017/S174392130600809X
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Abstract

We have conducted a survey of X-ray sources in XMM-Newton observations of M31, examining their power density spectra (PDS) and spectral energy distributions (SEDs). Our automated source detection yielded 535 good X-ray sources; to date, we have studied 225 of them. In particular, we examined the PDS because low mass X-ray binaries (LMXBs) exhibit two distinctive types of PDS. At low accretion rates, the PDS is characterised by a broken power law, with the spectral index changing from ∼0 to ∼1 at some frequency in the range ∼0.01-1 Hz; we refer to such PDS as Type A. At higher accretion rates, the PDS is described by a simple power law; we call these PDS Type B. Of the 225 sources studied to date, 75 exhibit Type A variability, and are almost certainly LMXBs, while 6 show Type B but not Type A, and are likely LMXBs. Of these 81 candidate LMXBs, 71 are newly identified in this survey; furthermore, they are mostly found near the centre of M31. Furthermore, most of the X-ray population in the disc are associated with the spiral arms, making them likely high mass X-ray binaries (HMXBs). In general these HMXBs do not exhibit Type A variability, while many central X-ray sources (LMXBs) in the same luminosity range do. Hence the PDS may distinguish between LMXBs and HMXBs in this luminosity range.

Item Type: Conference Item
ISSN: 1743-9213
Extra Information: Some of the symbols may not have transferred correctly into this bibliographic record and/or abstract.
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
eSTEeM
Item ID: 6035
Depositing User: Christopher Biggs
Date Deposited: 18 Dec 2006
Last Modified: 05 Mar 2014 10:27
URI: http://oro.open.ac.uk/id/eprint/6035
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