Issue |
EAS Publications Series
Volume 61, 2013
Gamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe
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Page(s) | 309 - 317 | |
Section | Chapter VII: Short GRBs | |
DOI | https://doi.org/10.1051/eas/1361049 | |
Published online | 22 July 2013 |
A.J. Castro-Tirado, J.Gorosabel and I.H. Park (eds) EAS Publications Series, 61 (2013) 309-317
Multi-Wavelength Observations of Short-Duration Gamma-Ray Bursts: Recent Results
1 Max-Planck-Institut für
extraterrestrische Physik, Giessenbachstraße, 85748
Garching,
Germany ;
e-mail: kann@tls-tautenburg.de
2 Universe Cluster, Technische
Universität München, Boltzmannstraße 2, 85748
Garching,
Germany ;
e-mail: kann@tls-tautenburg.de
3 Thüringer Landessternwarte
Tautenburg, Sternwarte 5, 07778
Tautenburg,
Germany ;
e-mail: kann@tls-tautenburg.de
The number of detections as well as significantly deep non-detections of optical/NIR afterglows of Type I (compact-object-merger population) Gamma-Ray Bursts (GRBs) has become large enough that statistically meaningful samples can now be constructed. I present within some recent results on the luminosity distribution of Type I GRB afterglows in comparison to those of Type II GRBs (collapsar population), the issue of the existence of jet breaks in Type I GRB afterglows, and the discovery of dark Type I GRBs.
© EAS, EDP Sciences 2013