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Identification of IGR J01217-7257 with the transient SMC pulsar XTE J0119-731 (SXP 2.16) using XMM-Newton.
- Source :
-
Monthly Notices of the Royal Astronomical Society . 2017, Vol. 470 Issue 2, p1971-1981. 11p. - Publication Year :
- 2017
-
Abstract
- The transient IGR J01217-7257 in the Small Magellanic Cloud was found to be in a new outburst during INTEGRALobservations. We triggered anXMM-Newton target of opportunity observation near outburst maximum, which lead to the discovery of X-ray pulsations with a period of 2.165 s. This period is very similar to that detected from XTE J0119-731, suggesting that both sources are identical. The pulse profile obtained from the EPIC-pn instrument is complex and highly energy dependent. Pulse-phase spectroscopy reveals variations in the spectral slope correlated with the changes in flux during the pulse, with the harder X-ray spectrum at pulse maximum and softer during minimum. Analysis of XMM-Newton reflection grating spectra reveals the presence of emission lines that suggest the presence of ionized material around the neutron star. By monitoring the system during its outburst with Swift/XRT we detected a possible transition from the accretor to the propeller stage. [ABSTRACT FROM AUTHOR]
- Subjects :
- *STARBURSTS
*BINARY pulsars
*X-ray binaries
*SMALL magellanic cloud
Subjects
Details
- Language :
- English
- ISSN :
- 00358711
- Volume :
- 470
- Issue :
- 2
- Database :
- Academic Search Index
- Journal :
- Monthly Notices of the Royal Astronomical Society
- Publication Type :
- Academic Journal
- Accession number :
- 124218133
- Full Text :
- https://doi.org/10.1093/mnras/stx1359