The Chandra Dust-scattering Halo of Galactic Center Transient Swift J174540.7-290015

• Main Authors: Corrales, L. R. (Author), Mon, B. (Author), Haggard, D. (Author), Garmire, G. (Author), Degenaar, N. (Author), Reynolds, M. (Author), Baganoff, Frederick K (Contributor)
• Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
• Format: Article
• Language: English
• Published: IOP Publishing, 2017-11-20T16:26:43Z.
• Subjects: Article
• Online Access: Get fulltext

 We report the detection of a dust-scattering halo around a recently discovered X-ray transient, Swift J174540.7-290015, which in early 2016 February underwent one of the brightest outbursts (F X ≈ 5 × 10[superscript -10] erg cm[superscript -2] s[superscript -1] ) observed from a compact object in the Galactic Center field. We analyze four Chandra images that were taken as follow-up observations to Swift discoveries of new Galactic Center transients. After adjusting our spectral extraction for the effects of detector pile-up, we construct a point-spread function for each observation an d compare it to the GC field before the outburst. We find residual surface brightness around Swift J174540.7-290015, which has a shape and temporal evolution consistent with the behavior expected from X-rays scattered by foreground dust. We examine the spectral properties of the source, which shows evidence that the object transitioned from a soft to hard spectral state as it faded below L X ∼ 10[superscript 36 ]erg s[superscript -1]. This behavior is consistent with the hypothesis that the object is a low-mass X-ray binary in the Galactic Center.