Haber F, Eger P, Pietsch W, Corbet RHD, Sasaki M (2008)
Publication Status: Published
Publication Type: Journal article
Publication year: 2008
Publisher: EDP SCIENCES S A
Book Volume: 485
Pages Range: 177-181
Journal Issue: 1
DOI: 10.1051/0004-6361:200809540
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.
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.
BibTeX: Download