A numerical approach for radiative cooling in relativistic outflows
- 31 January 2021
- journal article
- research article
- Published by Wiley in Astronomische Nachrichten
- Vol. 342 (1-2), 277-282
- https://doi.org/10.1002/asna.202113919
Abstract
No abstract availableKeywords
Funding Information
- Consejo Nacional de Ciencia y Tecnología (CVU332030)
This publication has 19 references indexed in Scilit:
- Inverse-Compton cooling in Klein-Nishina regime and gamma-ray burst prompt spectrumMonthly Notices of the Royal Astronomical Society, 2012
- On the multiwavelength emission from gamma ray burst afterglowsAstronomy & Astrophysics, 2009
- KLEIN–NISHINA EFFECTS ON OPTICALLY THIN SYNCHROTRON AND SYNCHROTRON SELF-COMPTON SPECTRUMThe Astrophysical Journal, 2009
- Spectra and Light Curves of Gamma-Ray Burst AfterglowsThe Astrophysical Journal, 1998
- Fokker-Planck Equations of Stochastic Acceleration: A Study of Numerical MethodsThe Astrophysical Journal Supplement Series, 1996
- Spectral properties of blast-wave models of gamma-ray burst sourcesThe Astrophysical Journal, 1994
- Radio Transients from Gamma-Ray BurstersThe Astrophysical Journal, 1993
- Gamma-ray bursts from stellar mass accretion disks around black holesThe Astrophysical Journal, 1993
- Are gamma-ray bursts optically thick?The Astrophysical Journal, 1986
- Gamma-ray bursters at cosmological distancesThe Astrophysical Journal, 1986