Delayed Afterglow Onset Interpreted as Baryon-Poor Viewing Angle

Details Delayed Afterglow Onset Interpreted as Baryon-Poor Viewing Angle Delayed Afterglow Onset Interpreted as Baryon-Poor Viewing Angle

2005-03-24

arxiv.org/abs/astro-ph/0503533v1

Astrophys.J. 628 (2005) L17-L20

Astronomy and Astrophysics

Astrophysics

Submitted to ApJ Letters February 24, 2005

Scientific paper

10.1086/431792

We have suggested previously that baryons in GRB fireballs infiltrate from
the surrounding walls that collimate the fireball. The efficiency $\epsilon_b$
for generating blast energy can then be angle dependent. Delayed onset of
afterglow can be interpreted as being due to a baryon-poor viewing angle.

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