XMM-Newton observations of the Small Magellanic Cloud: Be/X-ray binary pulsars active between October 2006 and June 2007

2008/06/25 by F. Haberl, P. Eger, W. Pietsch · 2 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Pulsars and Gravitational Waves Research #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810100

Accepted for publication in A&A, 22 pages, 12 figures

arxiv created 2008/06/25 · openalex publication_date 2008/07/28 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/01

Abstract

Aims. We analysed eight XMM-Newton observations toward the Small Magellanic Cloud (SMC), performed between October 2006 and June 2007, to investigate high mass X-ray binary systems.

Citations

• Least-squares frequency analysis of unequally spaced data
• Studies in astronomical time series analysis. II - Statistical aspects of spectral analysis of unevenly spaced data
• XMM-Newton observations of the Small Magellanic Cloud: X-ray outburst of the 6.85 s pulsar XTE J0103-728
• X-ray observations of Be/X-ray binaries in the SMC
• New XMM-Newton observations of supernova remnants in the Small Magellanic Cloud

Cited by

• Spectral and temporal properties of RX J0520.5-6932 (LXP 8.04) during a type-I outburst
• UPPER LIMITS ON PULSED RADIO EMISSION FROM THE 6.85 s X-RAY PULSAR XTE J0103–728 IN THE SMALL MAGELLANIC CLOUD

Related

• XMM-Newton observations of the Small Magellanic Cloud: X-ray outburst of the 6.85 s pulsar XTE J0103-728
• Discovery of 146.8 s pulsations from EP J005146.9-730930, a new transient Be/X-ray binary in the SMC
• New XMM-Newton observations of supernova remnants in the Small Magellanic Cloud
• X-ray source populations in the Magellanic Clouds
• X-Ray Binary Systems in the Small Magellanic Cloud