XMM-newton observations of the Small Magellanic Cloud: XMMUJ004814.1-731003, a 25.55 s Be/X-ray binary pulsar

Haber F, Eger P, Pietsch W, Corbet RHD, Sasaki M (2008)


Publication Status: Published

Publication Type: Journal article

Publication year: 2008

Journal

Publisher: EDP SCIENCES S A

Book Volume: 485

Pages Range: 177-181

Journal Issue: 1

DOI: 10.1051/0004-6361:200809540

Abstract

Aims: To investigate candidates for Be/X-ray binaries in the Small Magellanic Cloud (SMC), we observed a region around the emission nebula N19 with XMM-Newton in October 2006.
Methods: We analysed the EPIC data of the detected point sources to derive their spectral and temporal characteristics.
Results: We detected X-ray pulsations with a period of 25.550(2) s from the second-brightest source in the field, which we designate XMMU J004814.1-731003. The X-ray spectrum is well modelled by a highly absorbed (NH = 5 ×~1022 cm-2) power-law with photon index 1.33 ± 0.27. The precise X-ray position allows us to identify a Be star as the optical counterpart. XMMU J004814.1-731003 is located within the error circle of the transient ASCA source AX J0048.2-7309, but its position is inconsistent with that of the proposed optical counterpart of AX J0048.2-7309 (the emission line star [MA93] 215). It remains unclear if XMMU J004814.1-731003 is associated with AX J0048.2-7309. XMMU J004814.1-731003 might be identical to an RXTE pulsar that was discovered with a period of 25.5 s, but which is listed as a 51 s pulsar in the recent literature.

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APA:

Haber, F., Eger, P., Pietsch, W., Corbet, R.H.D., & Sasaki, M. (2008). XMM-newton observations of the Small Magellanic Cloud: XMMUJ004814.1-731003, a 25.55 s Be/X-ray binary pulsar. Astronomy & Astrophysics, 485(1), 177-181. https://doi.org/10.1051/0004-6361:200809540

MLA:

Haber, F., et al. "XMM-newton observations of the Small Magellanic Cloud: XMMUJ004814.1-731003, a 25.55 s Be/X-ray binary pulsar." Astronomy & Astrophysics 485.1 (2008): 177-181.

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