Low-Frequency Radio View Of The GRB030329 Blast Wave Deep Into Its Non-Relativistic Phase

Details Low-Frequency Radio View Of The GRB030329 Blast Wave Deep Into Its Non-Relativistic Phase Low-Frequency Radio View Of The GRB030329 Blast Wave Deep Into Its Non-Relativistic Phase

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.0506v&link_type=abstract

American Astronomical Society, HEAD meeting #10, #5.06

Physics

Scientific paper

We explore the physics behind one of the brightest radio afterglows ever, GRB030329, at late times when the blast wave is non-relativistic. We utilize our low-frequency radio observations with the Westerbork Synthesis Radio Telescope and the Giant Metrewave Radio Telescope, spanning an unprecedented temporal and spectral range, to determine the physical parameters of the blast wave and its surroundings. We compare our results with the ones from VLBI studies of the image size evolution and constrain the possible emission coming from a counter jet. Furthermore, we explore the potential of a new generation of low-frequency radio telescopes, like the Low Frequency Array, to study GRB afterglow physics.

Affiliated with

Also associated with

No associations

Rating

Low-Frequency Radio View Of The GRB030329 Blast Wave Deep Into Its Non-Relativistic Phase does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Low-Frequency Radio View Of The GRB030329 Blast Wave Deep Into Its Non-Relativistic Phase, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Low-Frequency Radio View Of The GRB030329 Blast Wave Deep Into Its Non-Relativistic Phase will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-958003