Constraints on the synchrotron self-Compton mechanism of TeV gamma ray emission from the Milagro TeV source MGRO J2019+37 within the pulsar wind nebula scenario-Reference-Cited by-同舟云学术

Constraints on the synchrotron self-Compton mechanism of TeV gamma ray emission from the Milagro TeV source MGRO J2019+37 within the pulsar wind nebula scenario

Published:2015-03 Issue: Volume:5-6 Page:9-14
ISSN:2214-4048
Container-title:Journal of High Energy Astrophysics
language:en
Short-container-title:Journal of High Energy Astrophysics

Author:

Saha Lab^ORCID,Bhattacharjee Pijushpani

Publisher

Elsevier BV

Subject

Astronomy and Astrophysics,Space and Planetary Science

Reference24 articles.

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4. Spectrum and morphology of the two brightest Milagro sources in the Cygnus region: MGRO J2019+37 and MGRO J2031+41;Abdo;Astrophys. J.,2012

5. Very High Energy Cosmic Gamma Radiation: A Crucial Window on the Extreme Universe;Aharonian,2004

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