SIMBAD references

2005MNRAS.364..455C - Mon. Not. R. Astron. Soc., 364, 455-461 (2005/December-1)

Discovery and study of the accreting pulsar 2RXP J130159.6-635806.

CHERNYAKOVA M., LUTOVINOV A., RODRIGUEZ J. and REVNIVTSEV M.

Abstract (from CDS):

We report on analysis of the poorly studied source 2RXP J130159.6-635806 at different epochs with ASCA, BeppoSAX, XMM-Newton and INTEGRAL. The source shows coherent X-ray pulsations at a period ∼700 s with an average spin-up rate of about. A broad-band (1-60 keV) spectral analysis of 2RXP J130159.6-635806 based on almost simultaneous XMM-Newton and INTEGRAL data demonstrates that the source has a spectrum typical of an accretion-powered X-ray pulsar, i.e. an absorbed power law with a high-energy cut-off with a photon index Γ∼ 0.5-1.0 and a cut-off energy of ∼25 keV. The long-term behaviour of the source, its spectral and timing properties, tend to indicate a high-mass X-ray binary with a Be companion. We also report on the identification of the likely infrared counterpart to 2RXP J130159.6-635806. The interstellar reddening does not allow us to strongly constrain the spectral type of the counterpart. The latter is, however, consistent with a Be star, the kind of which is often observed in accretion-powered X-ray pulsars.

Abstract Copyright: 2005 The Authors. Journal compilation © 2005 RAS

Journal keyword(s): pulsars: individual: 2RXP J130159.6-635806 - gamma-rays: observations - X-rays: binaries - X-rays: individual: 2RXP J130159.6-635806

Simbad objects: 10

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2005MNRAS.364..455C and select 'bookmark this link' or equivalent in the popup menu


2020.01.23-18:16:13

© Université de Strasbourg/CNRS

    • Contact