SIMBAD references

2008MNRAS.386L..10K - Mon. Not. R. Astron. Soc., 386, L10-L14 (2008/May-1)

Discovery of X-ray pulsations from the HMXB source AXJ1749.1-2733.

KARASEV D.I., TSYGANKOV S.S. and LUTOVINOV A.A.

Abstract (from CDS):

We are reporting the discovery of X-ray pulsations from the source AXJ1749.1-2733 with the period of ∼132 s based on the XMM-Newton data obtained in 2007 March. The observed pulse profile has a double-peaked structure with the pulse fraction of about 25-30 per cent in the 3-10 keV energy band. We have also found that a periodicity with practically the same period has been detected from the source by the IBIS telescope onboard the INTEGRAL observatory during an outburst on 2003 September 9 in the 20-50 keV energy band. Due to the double-peaked pulse profile, there is an additional peak on both periodograms of ∼66s; therefore we have also investigated the possibility that the last value is the true pulse period. The source spectrum obtained by the XMM-Newton observatory in the soft energy band is being heavily absorbed (NH≃ 2x1023/cm2) due to a strong intrinsic absorption in the binary system that leads to the conclusion that AXJ1749.1-2733 is a new transient X-ray pulsar in the high-mass X-ray binary system.

Abstract Copyright: ©2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): pulsars: individual: AXJ1749.1-2733 - X-ray: binaries

CDS comments: In Chap.5: AXJ1749.2-2733 is a misprint for AXJ1749.1-2733

Simbad objects: 4

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2021.02.26-23:28:52

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