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Katagiri, H.; Sugiyama, S.; Ackermann, M.; Ballet, J.; Casandjian, J. M.; Hanabata, Y.; Hewitt, J. W.; Kerr, M.; Kubo, H.; Lemoine-Goumard, M.; Ray, P. S.
The Astrophysical journal, 11/2016, Letnik: 831, Številka: 1Journal Article
ABSTRACT We present an analysis of the gamma-ray measurements by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope in the region of the supernova remnant (SNR) Monoceros Loop (G205.5+0.5). The brightest gamma-ray peak is spatially correlated with the Rosette Nebula, which is a molecular cloud complex adjacent to the southeast edge of the SNR. After subtraction of this emission by spatial modeling, the gamma-ray emission from the SNR emerges, which is extended and fit by a Gaussian spatial template. The gamma-ray spectra are significantly better reproduced by a curved shape than a simple power law. The luminosities between 0.2 and 300 GeV are erg s−1 for the SNR and erg s−1 for the Rosette Nebula, respectively. We argue that the gamma-rays likely originate from the interactions of particles accelerated in the SNR. The decay of neutral pions produced in nucleon-nucleon interactions of accelerated hadrons with interstellar gas provides a reasonable explanation for the gamma-ray emission of both the Rosette Nebula and the Monoceros SNR.
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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