2011A&A...526A.121D


C.D.S. - SIMBAD4 rel 1.7 - 2020.01.29CET02:56:35

2011A&A...526A.121D - Astronomy and Astrophysics, volume 526A, 121-121 (2011/2-1)

Gamma-ray bursts afterglows with energy injection from a spinning down neutron star.

DALL'OSSO S., STRATTA G., GUETTA D., COVINO S., DE CESARE G. and STELLA L.

Abstract (from CDS):

We investigate a model for the shallow decay phases of gamma-ray burst (GRB) afterglows discovered by Swift/XRT in the first hours following a GRB event. In the context of the fireball scenario, we consider the possibility that long-lived energy injection from a millisecond spinning, ultramagnetic neutron star (magnetar) powers afterglow emission during this phase. We consider the energy evolution in a relativistic shock that is subject to both radiative losses and energy injection from a spinning down magnetar in spherical symmetry. We model the energy injection term through magnetic dipole losses and discuss an approximate treatment for the dynamical evolution of the blastwave. We obtain an analytic solution for the energy evolution in the shock and associated lightcurves. To fully illustrate the potential of our solution we calculate lightcurves for a few selected X-ray afterglows observed by Swift and fit them using our theoretical lightcurves. Our solution naturally describes in a single picture the properties of the shallow decay phase and the transition to the so-called normal decay phase. In particular, we obtain remarkably good fits to X-ray afterglows for plausible parameters of the magnetar. Even though approximate, our treatment provides a step forward with respect to previously adopted approximations and provides additional support of the idea that a millisecond spinning (1-3ms), ultramagnetic (B∼1014-1015G) neutron star loosing spin energy through magnetic dipole radiation can explain the luminosity, durations and shapes of X-ray GRB afterglows.

Abstract Copyright:

Journal keyword(s): gamma-ray burst: general - X-rays: bursts - shock waves - stars: magnetars - relativistic processes

Simbad objects: 2

goto Full paper

goto View the reference in ADS

Number of rows : 2

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 GRB 060729 gB 06 21 31.850 -62 22 12.69           ~ 243 0
2 GRB 050801 gB 13 36 35.000 -21 55 41.00 15.03 15.82 15.46     ~ 138 0

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2011A&A...526A.121D and select 'bookmark this link' or equivalent in the popup menu


2020.01.29-02:56:35

© Université de Strasbourg/CNRS

    • Contact