2010/02/28 by Daniel Castro, Patrick Slane · 1 citation
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Cosmic ray #Dark Matter and Cosmic Phenomena #Fermi Gamma-ray Space Telescope #Gamma-ray bursts and supernovae #Maser #Molecular cloud #Physics #Spitzer Space Telescope #Supernova #Supernova remnant #Telescope #astro-ph.HE
paper · pdf · doi:10.1088/0004-637x/717/1/372
8 pages, 8 figures, 2 tables, accepted for publication in ApJ
arxiv created 2010/06/09 · openalex publication_date 2010/06/11 · arxiv updated 2015/05/18 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We report the detection of γ-ray emission coincident with four supernova remnants (SNRs) using data from the Large Area Telescope on board the Fermi Gamma-ray Space Telescope . G349.7+0.2, CTB 37A, 3C 391, and G8.7−0.1 are SNRs known to be interacting with molecular clouds, as evidenced by observations of hydroxyl (OH) maser emission at 1720 MHz in their directions. SNR shocks are expected to be sites of cosmic-ray acceleration, and clouds of dense material can provide effective targets for production of γ-rays from π 0 decay. The observations reveal unresolved sources in the direction of G349.7+0.2, CTB 37A, and 3C 391, and a possibly extended source coincident with G8.7−0.1, all with significance levels greater than 10σ.