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Behind the dust curtain: the spectacular case of GRB 160623A

Journal Article · · Monthly Notices of the Royal Astronomical Society
 [1];  [2];  [1];  [3];  [1];  [4];  [5];  [1];  [6]
  1. INAF – IASF Milano, Milano (Italy)
  2. INAF – IASF Milano, Milano (Italy); Scuola Univ. Superiore IUSS Pavia, Pavia (Italy); Istituto Nazionale di Fisica Nucleare, Pavia (Italy)
  3. Stanford Univ., Stanford, CA (United States). SLAC National Accelerator Lab.
  4. Univ. of Amsterdam, Amsterdam (The Netherlands)
  5. SRON Netherlands Institute for Space Research, Utrecht (The Netherlands)
  6. Univ. of Zagreb, Zagreb (Croatia)
Here, we report on the X-ray dust-scattering features observed around the afterglow of the gamma-ray burst GRB 160623A. With an XMM–Newton observation carried out ~2 d after the burst, we found evidence of at least six rings, with angular size expanding between ~2 and 9 arcmin, as expected for X-ray scattering of the prompt gamma-ray burst (GRB) emission by dust clouds in our Galaxy. From the expansion rate of the rings, we measured the distances of the dust layers with extraordinary precision: 528.1 ± 1.2, 679.2 ± 1.9, 789.0 ± 2.8, 952 ± 5, 1539 ± 20 and 5079 ± 64 pc. A spectral analysis of the ring spectra, based on an appropriate dust-scattering model (BARE-GR-B) and the estimated burst fluence, allowed us to derive the column density of the individual dust layers, which are in the range 7 × 1020–1.5 × 1022 cm–2. The farthest dust layer (i.e. the one responsible for the smallest ring) is also the one with the lowest column density and it is possibly very extended, indicating a diffuse dust region. The properties derived for the six dust layers (distance, thickness and optical depth) are generally in good agreement with independent information on the reddening along this line of sight and on the distribution of molecular and atomic gas.
Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1419258
Journal Information:
Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 2 Vol. 472; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English

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Cited By (1)

The X-Ray Variable Sky as Seen by MAXI: The Future of Dust-echo Tomography with Bright Galactic X-Ray Bursts journal April 2019

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