XMM-Newton discovery of transient 285.4 s X-ray pulsar XMMU J013359.5+303634 in M33
Abstract
I report on the discovery and analysis of the first transient X-ray pulsar detected in the Local Group galaxy M33. The 2010 July-August deep XMM-Newton observations of M33 fields revealed a new bright X-ray source XMMU J013359.5+303634 exhibiting pulsations with a period P ∼ 285.4 s and pulsed fraction ∼47 per cent in the 0.3-10 keV energy range. The pulse phase averaged spectrum of XMMU J013359.5+303634 is typical of X-ray pulsars and can be fitted with an absorbed simple power-law model of photon index Γ ∼ 1.2 in the 0.3-10 keV energy band. The search for an optical counterpart did not yield any stellar object brighter than 20 mag, suggesting that XMMU J013359.5+303634 is not a Galactic foreground object and almost certainly belongs to M33. Assuming the distance of 817 kpc, the maximum observed luminosity of the source in the 0.3-10 keV energy range is ∼1.4 × 1037 erg s-1, at least 20 times higher than quiescent luminosity. The brightest optical object inside the error circle of XMMU J013359.5+303634 has a visual magnitude of 20.9 and properties consistent with being an early B V star when placed at a distance of M33. Based on the X-ray pulsations and spectrum, transient behaviour and possible early B class optical counterpart, XMMU J013359.5+303634 can be classified as another extragalactic Be/X-ray binary candidate.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- November 2013
- DOI:
- 10.1093/mnras/stt1518
- arXiv:
- arXiv:1209.2780
- Bibcode:
- 2013MNRAS.435.3326T
- Keywords:
-
- X-rays: binaries;
- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Astrophysics of Galaxies;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- 7 pages, 6 figures. Accepted for publication in MNRAS. Updated to match the accepted version