Thermal Components in the Early X-Ray Afterglows of GRBs: Likely Cocoon Emission and Constraints on the Progenitors

Monthly Notices of the Royal Astronomical Society - United Kingdom
doi 10.1093/mnras/stx2920
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Oxford University Press (OUP)

Related search

Thermal Emission in Grbs: The Case of GRB 090618

International Journal of Modern Physics: Conference Series
2013English

Statistical Connection Between the Prompt and X-Ray Afterglow Emission of Swift Detected GRBs

2012English

The Soft X-Ray Landscape of Gamma-Ray Bursts: Thermal Components

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2011English

Early Rebrightenings of X-Ray Afterglows From Ring-Shaped GRB Jets

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2010English

X-Ray Emission Lines in GRB Afterglows: Evidence for a Two-Component Jet Model

Chinese Journal of Astronomy and Astrophysics
2005English

Low-Mass X-Ray Binaries as the Source of the Very Soft X-Ray Emission in the X-Ray–faintest Early-Type Galaxies

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1998English

X-Ray Behaviour of GRBs Detected by INTEGRAL/JEM-X

2013English

Erratum: Thermal X-Ray Emission From Supernova 1987A

Nature
Multidisciplinary
1987English

Non-Thermal Hard X-Ray Emission From M87

2009English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy