skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Radio observations of GRB 100418a: Test of an energy injection model explaining long-lasting GRB afterglows

Journal Article · · Astrophysical Journal
;  [1];  [2]; ; ;  [3];  [4];  [5];  [6]
  1. Shanghai Astronomical Observatory, 80 Nandan Road, Xujiahui, Shanghai 200030 (China)
  2. National Center for Radio Astrophysics, Tata Institute of Fundamental Research, Pune (India)
  3. International Centre for Radio Astronomy Research, Curtin University, Bentley 6102, WA (Australia)
  4. Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM 87131 (United States)
  5. National Radio Astronomy Observatory, P.O. Box 0, Socorro, NM 87801 (United States)
  6. CSIRO Astronomy and Space Science, PO Box 76, Epping, NSW (Australia)

We present the results of our radio observational campaign of gamma-ray burst (GRB) 100418a, for which we used the Australia Telescope Compact Array, the Very Large Array, and the Very Long Baseline Array. GRB 100418a was a peculiar GRB with unusual X-ray and optical afterglow profiles featuring a plateau phase with a very shallow rise. This observed plateau phase was believed to be due to a continued energy injection mechanism that powered the forward shock, giving rise to an unusual and long-lasting afterglow. The radio afterglow of GRB 100418a was detectable several weeks after the prompt emission. We conducted long-term monitoring observations of the afterglow and attempted to test the energy injection model advocating that the continuous energy injection is due to shells of material moving at a wide range of Lorentz factors. We obtained an upper limit of γ < 7 for the expansion rate of the GRB 100418a radio afterglow, indicating that the range-of-Lorentz factor model could only be applicable for relatively slow-moving ejecta. A preferred explanation could be that continued activity of the central engine may have powered the long-lasting afterglow.

OSTI ID:
22348467
Journal Information:
Astrophysical Journal, Vol. 779, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English

Similar Records

THE LATE PEAKING AFTERGLOW OF GRB 100418A
Journal Article · Tue Feb 01 00:00:00 EST 2011 · Astrophysical Journal · OSTI ID:22348467

The origin of the plateau and late rebrightening in the afterglow of GRB 120326A
Journal Article · Sun Apr 20 00:00:00 EDT 2014 · Astrophysical Journal · OSTI ID:22348467

Early GRB Afterglows from Reverse Shocks in Ultra-relativistic, Long-lasting Winds
Journal Article · Tue Jan 31 00:00:00 EST 2017 · The Astrophysical Journal (Online) · OSTI ID:22348467