Date:
Tue, 16/02/201612:30-13:30
Location:
Kaplun building' Room No. 200
Lecturer: Dr. Christopher Irwin
Affiliation: The University of Virginia
Abstract:
We consider a model for the long-duration, low-
luminosity gamma-ray burst GRB 060218 that
plausibly accounts for multiwavelength
observations to day 20. The components of our
model are: (1) a long-lived (t ~ 3000 s) central
engine and accompanying low-luminosity (L ~
1e47 erg/s), mildly relativistic jet; (2) a low-
mass (~ 1e-2 Msun ) envelope surrounding the
progenitor star; and (3) a modest amount of
dust (A_V ~ 0.1) in the circumstellar or
interstellar environment. Blackbody emission
from the transparency radius in a low-power jet
outflow can fit the prompt thermal X-ray
emission, and the prompt nonthermal X-rays
and gamma-rays may be produced via Compton
scattering of thermal photons from hot leptons
in the jet interior or the external shocks. The
later mildly relativistic phase of this outflow can
produce the radio emission via synchrotron
radiation from the forward shock. Meanwhile,
interaction of the associated SN 2006aj with a
circumstellar envelope extending to ~ 10 cm
can explain the early optical peak. The X-ray
afterglow can be interpreted as a light echo of
the prompt emission from dust at ~ 30 pc. Our
model is a plausible alternative to that of Nakar,
who recently proposed shock breakout of a jet
smothered by an extended envelope as the
source of prompt emission. Both our results and
Nakar's suggest that ultra-long bursts such as
GRB 060218 and GRB 100316D may originate
from unusual progenitors with extended
circumstellar envelopes, and that a jet is
necessary to decouple the prompt high-energy
emission from the supernova. We discuss the
advantages and drawbacks of each model, and
consider implications for the classification of
long-duration gamma-ray transients.
Additional details of the upcoming Astrophysics'
seminars can be found on the following link.
האירוע הזה כולל שיחת וידאו ב-Google Hangouts.
הצטרף: https://hangouts.google.com/hangouts/_/mail.huji.ac.il/astrophysics?hceid=bWFpbC5odWppLmFjLmlsX2c0czhydDlpcmhwZzRvdGNybWIzZGFqcjdvQGdyb3VwLmNhbGVuZGFyLmdvb2dsZS5jb20.pi8vfmu9ppf58cf9k1j1i7cer4&hs=121