2013MNRAS.434.3463Z

Query : 2013MNRAS.434.3463Z

2013MNRAS.434.3463Z - Mon. Not. R. Astron. Soc., 434, 3463-3468 (2013/October-1)

Long-term X-ray emission from Swift J1644+57.

ZOU Y.C., WANG F.Y. and CHENG K.S.

Abstract (from CDS):

The X-ray emission from Swift J1644+57 is not steadily decreasing; instead, it shows multiple pulses with declining amplitudes. We model the pulses as reverse shocks from collisions between the late ejected shells and the externally shocked material, which is decelerated while sweeping the ambient medium. The peak of each pulse is taken as the maximum emission of each reverse shock. With a proper set of parameters, the envelope of peaks in the light curve as well as the spectrum can be modelled well.

Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)

Journal keyword(s): radiation mechanisms: non-thermal - X-rays: general

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 GRB 070311 gB 05 50 08.220 +03 22 29.40           ~ 68 0
2 NGC 5905 H2G 15 15 23.3280793632 +55 31 01.926808032   13.6       ~ 287 1
3 SWIFT J164449.3+573451 G 16 44 47.81184000 +57 35 00.7113480           ~ 533 0
4 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
5 GRB 071118 gB 19 58 51.77 +70 07 27.9           ~ 44 0

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