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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3581

Title: Multiwavelength study of the transient X-ray binary IGR J01583+6713
Authors: Kaur, Ramanpreet
Paul, Biswajit
Kumar, Brijesh
Sagar, Ram
Keywords: binaries: general
stars: emission-line
stars: individual: IGR J01583+6713
pulsars: general
X-rays: stars
Issue Date: May-2008
Publisher: Blackwell Publishing for the RAS
Citation: Monthly Notices of the Royal Astronomical Society, 2008, Vol.386, p2253
Abstract: We have investigated multiband optical photometric variability and stability of the Hα line profile of the transient X-ray binary IGR J01583+6713. We set an upper limit of 0.05 mag on photometric variations in the V band over a time-scale of three months. The Hα line is found to consist of non-Gaussian profile and quite stable for a duration of two months. We have identified the spectral type of the companion star to be B2 IVe while the distance to the source is estimated to be ~4.0 kpc. Along with the optical observations, we have also carried out analysis of X-ray data from three short observations of the source, two with the Swift-XRT and one with the RXTE-PCA. We have detected a variation in the absorption column density, from a value of 22.0 × 1022 cm-2 immediately after the outburst down to 2.6 × 1022 cm-2 four months afterwards. In the quiescent state, the X-ray absorption is consistent with the optical reddening measurement of E(B - V) = 1.46 mag. From one of the Swift observations, during which the X-ray intensity was higher, we have a possible pulse detection with a period of 469.2 s. For a Be X-ray binary, this indicates an orbital period in the range of 216-561 d for this binary system.
Description: Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)
URI: http://hdl.handle.net/2289/3581
ISSN: E-ISSN: 1365-2966
P-ISSN: 0035-8711
Alternative Location: http://adsabs.harvard.edu/abs/2008MNRAS.386.2253K
Copyright: 2008 RAS
Appears in Collections:Research Papers (A&A)

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