Tools
Tools
Cenko, SB, Frail, DA, Harrison, FA, Haislip, JB, Reichart, DE, Butler, NR, Cobb, BE, Cucchiara, A, Berger, E, Bloom, JS, Chandra, P, Fox, DB, Perley, DA, Prochaska, JX, Filippenko, AV, Glazebrook, K, Ivarsen, KM, Kasliwal, MM, Kulkarni, SR, Lacluyze, AP , Lopez, S, Morgan, AN, Pettini, M and Rana, VR (2011) Afterglow observations of Fermi large area telescope gamma-ray bursts and the emerging class of hyper-energetic events. The Astrophysical Journal, 732 (1). ISSN 1538-4357
|
Text
Cenko_2011_ApJ_732_29.pdf - Published Version Download (1MB) | Preview |
Abstract
We present broadband (radio, optical, and X-ray) light curves and spectra of the afterglows of four long-duration gamma-ray bursts (GRBs;GRBs 090323, 090328, 090902B, and 090926A) detected by the Gamma-Ray Burst Monitor and Large Area Telescope (LAT) instruments on the Fermi satellite. With its wide spectral bandpass, extending to GeV energies, Fermi is sensitive to GRBs with very large isotropic energy releases (1054 erg). Although rare, these events are particularly important for testing GRB central-engine models. When combined with spectroscopic redshifts, our afterglow data for these four events are able to constrain jet collimation angles, the density structure of the circumburst medium, and both the true radiated energy release and the kinetic energy of the outflows. In agreement with our earlier work, we find that the relativistic energy budget of at least one of these events (GRB090926A) exceeds the canonical value of 1051erg by an order of magnitude. Such energies pose a severe challenge for models in which the GRB is powered by a magnetar or a neutrino-driven collapsar, but remain compatible with theoretical expectations for magnetohydrodynamical collapsar models (e.g., the Blandford-Znajek mechanism). Our jet opening angles (θ) are similar to those found for pre-Fermi GRBs, but the large initial Lorentz factors (Γ0) inferred from the detection of GeV photons imply θΓ0 ≈ 70-90, values which are above those predicted in magnetohydrodynamic models of jet acceleration. Finally, we find that these Fermi-LAT events preferentially occur in a low-density circumburst environment, and we speculate that this might result from the lower mass-loss rates of their lower-metallicity progenitor stars. Future studies of Fermi-LAT afterglows at radio wavelengths with the order-of-magnitude improvement in sensitivity offered by the Extended Very Large Array should definitively establish the relativistic energy budgets of these events. © 2011. The American Astronomical Society. All rights reserved.
| Item Type: | Article |
|---|---|
| Uncontrolled Keywords: | 0201 Astronomical And Space Sciences, 0305 Organic Chemistry, 0306 Physical Chemistry (Incl. Structural) |
| Subjects: | Q Science > QB Astronomy Q Science > QC Physics Q Science > QD Chemistry |
| Divisions: | Astrophysics Research Institute |
| Publisher: | American Astronomical Society |
| Date Deposited: | 22 May 2017 11:27 |
| Last Modified: | 20 Apr 2022 09:46 |
| DOI or ID number: | 10.1088/0004-637X/732/1/29 |
| URI: | https://researchonline.ljmu.ac.uk/id/eprint/6491 |
 |
View Item |