[vsnet-grb-info 4270] GRB 070129: dust-scattered X-ray halo detected
by Swift/XRT
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Wed Jan 31 23:31:41 JST 2007
TITLE: GCN CIRCULAR
NUMBER: 6065
SUBJECT: GRB 070129: dust-scattered X-ray halo detected by Swift/XRT
DATE: 07/01/31 14:31:35 GMT
FROM: Sandro Mereghetti at IASF/CNR <sandro at iasf-milano.inaf.it>
G. Vianello (INAF, IASF-Milano & Univ. dell'Insubria), A. Tiengo, S.
Mereghetti (INAF, IASF-Milano) report:
We discovered a faint dust scattering halo in the Swift XRT Photon
Counting mode data of GRB 070129. The halo consists of a partial ring of
radius ~2 arcmin located to the North-West of the GRB afterglow position.
Analysis of the dynamical image (see Tiengo & Mereghetti 2006 A&A 449,
203) covering the period from T0+4700s to T0+7300s (where T0 is the BAT
trigger time, as reported in GCN 6053) indicates that the halo is
expanding and leads to an estimate of ~300 pc for the distance of the dust
layer responsible for the scattering.
Dust maps (Schlegel, Finkbeiner, & Davis 1998, ApJ, 500, 525) show a
diffuse structure in the direction indicated by the partial ring, and a
total Galactic extinction of A_v~0.4.
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