EDP Sciences
Free Access
Volume 403, Number 3, June I 2003
Page(s) 901 - 916
Section Galactic structure and dynamics
DOI https://doi.org/10.1051/0004-6361:20030420
Published online 23 May 2003

A&A 403, 901-916 (2003)
DOI: 10.1051/0004-6361:20030420

XMM-Newton observations of High Mass X-ray Binaries in the SMC

M. Sasaki, W. Pietsch and F. Haberl

Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, Postfach 1312, 85741 Garching, Germany
(Received 11 December 2002 / Accepted 17 March 2003 )

Based on XMM-Newton EPIC data of four pointings towards the Small Magellanic Cloud (SMC), results on timing and spectral analyses of 16 known high mass X-ray binaries (HMXBs) and HMXB candidates in the SMC are presented. We confirm the pulse periods of four sources which were known to show pulsations. In addition, two new X-ray pulsars are discovered: XMMU J005605.2-722200 with $P_{\rm pulse} = 140.1\pm0.3$ s and RX J0057.8-7207 with $P_{\rm pulse} = 152.34\pm0.05$ s. Due to the low Galactic foreground absorption, X-ray binary systems in the Magellanic Clouds are well suited for studies of the soft component in their X-ray spectrum. Spectral analysis reveals soft emission besides a power law component in the spectra of three sources. The existence of emission lines in at least one of them corroborates the thermal nature of this emission with temperatures of 0.2-0.3 keV and heavy element abundances lower than solar. For the HMXB SMC X-2 which was in a low luminosity state, we determine a flux upper limit of $1.5\times 10^{-14}$ erg cm -2 s -1 (0.3-10.0 keV). Furthermore, two new sources (XMMU J005735.7-721932 and XMMU J010030.2-722035) with hard spectrum and emission line objects as likely optical counterparts are proposed as new X-ray binary candidates.

Key words: X-rays: galaxies -- X-rays: binaries -- stars: neutron -- Magellanic Clouds

Offprint request: M. Sasaki, msasaki@cfa.harvard.edu

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© ESO 2003

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