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A&A 437, 899-904 (2005)
DOI: 10.1051/0004-6361:20053060
Discovery of multiple ultra-luminous X-ray sources in the galaxy KUG 0214-057
M. G. Watson1, T. P. Roberts1, M. Akiyama2 and Y. Ueda31 Department of Physics & Astronomy, University of Leicester, Leicester, LE1 7RH, UK
e-mail: mgw@star.le.ac.uk
2 Subaru Telescope, National Astronomical Observatory of Japan, 650 North A'ohoku Place, Hilo, HI 96720, USA
3 Institute of Space and Astronautical Science, Sagamihara, Kanagawa 229-8510, Japan
(Received 21 December 2004 / Accepted 6 April 2005 )
Abstract
We report the serendipitous discovery of several
unresolved X-ray sources lying in the prominent spiral arms of the galaxy
KUG 0214-057
in XMM-Newton observations. The location of
these
X-ray sources strongly suggests that at least three, and possibly four, of
these may be physically related to the galaxy. The luminosity of each
of these sources at the distance of KUG 0214-057 is >
(0.3-10 keV), making each a strong candidate
ultraluminous
X-ray source (ULX). Using the ULXs objects as a metric implies that this
relatively low-mass
galaxy may be experiencing rather intense starburst activity. The
serendipitous discovery of these ULXs objects suggests that such objects
are not a negligible component of the overall extragalactic X-ray source
population.
Key words: X-rays: galaxies -- galaxies: starburst
SIMBAD Objects
© ESO 2005
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