Issue |
A&A
Volume 461, Number 1, January I 2007
|
|
---|---|---|
Page(s) | L9 - L12 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:20066527 | |
Published online | 20 November 2006 |
Letter to the Editor
A Wolf-Rayet/black-hole X-ray binary candidate in NGC 300
1
XMM-Newton Science Operations Centre, ESAC, European Space Agency, Apartado 50727, 28080 Madrid, Spain e-mail: scarpano@sciops.esa.int
2
Dr. Remeis Sternwarte, Astronomisches Institut der FAU Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany
3
Isaac Newton Group of Telescopes, 38700 Santa Cruz de La Palma, Spain
Received:
9
October
2006
Accepted:
6
November
2006
Context.Wolf Rayet/black hole binaries are believed to exist as a later evolutionary product of high-mass X-ray binaries. Hundreds of such binaries may exist in galaxies, but only a few of them are close enough to be observed as X-ray binaries. Only a couple of candidates have been reported so far.
Aims.Based on XMM-Newton observations, we report the positional coincidence of the brightest X-ray source in NGC 300 (NGC 300 X-1) with a Wolf-Rayet candidate. Temporal and spectral analysis of the X-ray source is performed.
Methods.We determine an accurate X-ray position of the object, and derive light curves, spectra and flux in four XMM-Newton observations.
Results.The positions of the X-ray source and the helium
star candidate coincide within ±
. The X-ray
light curves show irregular variability. During one XMM-Newton
observation, the flux increased by about a factor of ten in 10 h. The spectrum can be modelled
by a power-law with
with additional relatively weak line emission,
notably around 0.95 keV. The mean observed (absorbed) luminosity in the
0.2–10 keV band is ~2
.
Conclusions.NGC 300 X-1 is
a good candidate for a Wolf-Rayet/black-hole X-ray binary: its
position coincides with a Wolf-Rayet candidate and the unabsorbed
X-ray luminosity reached
,
suggesting the presence of a black hole.
Key words: galaxies: individual: NGC 300 / X-rays: binaries / stars: Wolf-Rayet
© ESO, 2006
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