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A&A 430, L45-L48 (2005)
DOI: 10.1051/0004-6361:200400128
Letter
XMM-Newton detection of type I X-ray bursts in M 31
W. Pietsch and F. HaberlMax-Planck-Institut für extraterrestrische Physik, 85741 Garching, Germany
e-mail: wnp@mpe.mpg.de
(Received 2 December 2004 / Accepted 15 December 2004)
Abstract
We searched for X-ray bursts in XMM-Newton
archival data of X-ray sources in
M 31
globular clusters (GCs) and
GC candidates. We detected two bursts simultaneously in EPIC pn and MOS
detectors and some more candidates in EPIC pn. The energy distribution
of the burst photons and the intrinsic luminosity
during the peak of the bursts indicate
that at least the strongest burst was a type I radius expansion burst.
The bursts identify the
sources as neutron star low mass X-ray binaries in
M 31
.
The type I X-ray bursts in
M 31
are the first
detected outside the Milky Way and show that with the help of XMM-Newton
X-ray bursts can be used to classify neutron star low mass X-ray
binaries in Local Group galaxies.
Key words: galaxies: individual: M 31 -- X-rays: galaxies -- galaxies: star clusters -- X-rays: binaries -- X-rays: bursts
SIMBAD Objects
© ESO 2005
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