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A view of supernova remnant CTB 37A with the Fermi Gamma-ray Space Telescope

2011/08/13 by T. J. Brandt · 14 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Cosmic ray #Dark Matter and Cosmic Phenomena #Fermi Gamma-ray Space Telescope #Gamma ray #Gamma-ray bursts and supernovae #Physics #Spitzer Space Telescope #Supernova #Supernova remnant #Telescope #astro-ph.HE

paper · pdf · doi:10.1016/j.asr.2011.07.021

published in Advances in Space Research 51(2), 247-252 (Elsevier BV) · published in Advances in Space Research

openalex publication_date 2011/08/13 · arxiv created 2013/05/01 · arxiv updated 2013/05/02 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Supernovae and their remnants have long been favored as cosmic ray ac- celerators. Recent data from the Fermi Gamma-ray Space Telescope has given us an improved window into such sources, including the remnant CTB 37A. Using the Fermi Large Area Telescope, we found significant gamma-ray emission coincident with the remnant, which also emits in radio, X-ray, and very high energy gamma-rays. We modeled the multiwavelength spectrum using a combination of hadronic and leptonic emission with reasonable parameter values and determined that CTB 37A is a potential cosmic ray accelerator commensurate with direct observations. By assembling statistically significant populations of such objects, we will be able to more fully illuminate the mystery of cosmic ray origins.

Citations