Observation of supernova remnant IC 443 with the Fermi Large Area Telescope

Abdo, A. A.

doi:10.1088/0004-637X/712/1/459

Title: Observation of supernova remnant IC 443 with the Fermi Large Area Telescope

Journal Article · Wed Mar 03 00:00:00 EST 2010 · The Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/712/1/459· OSTI ID:1357575

Abdo, A. A. ^[1]

Naval Research Lab. (NRL), Washington, DC (United States); National Academy of Sciences, Washington, DC (United States); et al.

Here, we report observation of the supernova remnant (SNR) IC 443 (G189.1+3.0) with the Fermi Gamma-ray Space Telescope Large Area Telescope (LAT) in the energy band between 200 MeV and 50 GeV. IC 443 is a shell-type SNR with mixed morphology located off the outer Galactic plane where high-energy emission has been detected in the X-ray, GeV and TeV gamma-ray bands. Past observations suggest IC 443 has been interacting with surrounding interstellar matter. Proximity between dense shocked molecular clouds and GeV-TeV gamma-ray emission regions detected by EGRET, MAGIC, and VERITAS suggests an interpretation that cosmic-ray (CR) particles are accelerated by the SNR. We accurately characterize the gamma-ray emission produced by the CRs accelerated at IC 443 using the high gamma-ray statistics and broad energy coverage provided by the LAT. The emission region is extended in the energy band with θ₆₈ = 0$$°\atop{.}$$27 ± 0fdg01(stat) ± 0$$°\atop{.}$$03(sys) for an assumed two-dimensional Gaussian profile and overlaps almost completely with the extended source region of VERITAS. Its centroid is displaced significantly from the known pulsar wind nebula (PWN) which suggests the PWN is not the major contributor in the present energy band. The observed spectrum changes its power-law slope continuously and continues smoothly to the MAGIC and VERITAS data points. Furthermore, the combined gamma-ray spectrum (200 MeV < 2 TeV) is reproduced well by decays of neutral pions produced by a broken power-law proton spectrum with a break around 70 GeV.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE

Contributing Organization:: Fermi LAT Collaboration

Grant/Contract Number:: AC02-76SF00515

OSTI ID:: 1357575

Journal Information:: The Astrophysical Journal, Vol. 712, Issue 1; ISSN 0004-637X

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 198 works

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Gamma-ray observations of the Be/pulsar binary 1A 0535+262 during a giant X-ray outburst Collaboration, Veritas; Acciari, V. A.; Aliu, E. arXiv https://doi.org/10.48550/arxiv.1103.3250	text	January 2011
Investigating the Cosmic-Ray Ionization Rate in the Galactic Diffuse Interstellar Medium through Observations of H3+ Indriolo, Nick; McCall, Benjamin J. arXiv https://doi.org/10.48550/arxiv.1111.6936	text	January 2011
Supernova remnants: the X-ray perspective Vink, Jacco arXiv https://doi.org/10.48550/arxiv.1112.0576	text	January 2011
Search for Dark Matter Satellites using the FERMI-LAT Collaboration, The Fermi LAT; Ackermann, M.; Albert, A. arXiv https://doi.org/10.48550/arxiv.1201.2691	text	January 2012
Fermi-LAT Observations of the Diffuse Gamma-Ray Emission: Implications for Cosmic Rays and the Interstellar Medium Collaboration, Lat arXiv https://doi.org/10.48550/arxiv.1202.4039	text	January 2012
Observational signatures of particle acceleration in supernova remnants Helder, E. A.; Vink, J.; Bykov, A. M. arXiv https://doi.org/10.48550/arxiv.1206.1593	text	January 2012
Diffuse Galactic Gamma Rays from Shock-Accelerated Cosmic Rays Dermer, Charles D. arXiv https://doi.org/10.48550/arxiv.1206.2899	text	January 2012
Analytic Solution for Self-regulated Collective Escape of Cosmic Rays from their Acceleration Sites Malkov, M. A.; Diamond, P. H.; Sagdeev, R. Z. arXiv https://doi.org/10.48550/arxiv.1207.4728	text	January 2012
HESS J1640-465 - an exceptionally luminous TeV gamma-ray supernova remnant Collaboration, H. E. S. S.; Abramowski, A.; Aharonian, F. arXiv https://doi.org/10.48550/arxiv.1401.4388	text	January 2014
Recombining Plasma in the Gamma-ray Emitting Mixed-Morphology Supernova Remnant 3C 391 Ergin, Tülün; Sezer, Aytap; Saha, Lab arXiv https://doi.org/10.48550/arxiv.1406.2179	text	January 2014
The origin of galactic cosmic rays Amato, Elena arXiv https://doi.org/10.48550/arxiv.1406.7714	text	January 2014
Global Distribution of Ionizing and Recombining Plasmas in the Supernova Remnant G290.1$-$0.8 Kamitsukasa, Fumiyoshi; Koyama, Katsuji; Uchida, Hiroyuki arXiv https://doi.org/10.48550/arxiv.1411.6809	text	January 2014
The supernova remnant W49B as seen with H.E.S.S. and Fermi-LAT Collaboration, H. E. S. S.; Abdalla, H.; Abramowski, A. arXiv https://doi.org/10.48550/arxiv.1609.00600	text	January 2016
3FHL: The Third Catalog of Hard Fermi-LAT Sources Collaboration, Lat arXiv https://doi.org/10.48550/arxiv.1702.00664	text	January 2017
NuSTAR Detection of a Hard X-ray Source in the Supernova Remnant - Molecular Cloud Interaction Site of IC 443 Zhang, Shuo; Tang, Xiaping; Zhang, Xiao arXiv https://doi.org/10.48550/arxiv.1805.08870	text	January 2018
The GeV emission in the field of the star-forming region W30 revisited Liu, Bing; Yang, Rui-zhi; Sun, Xiao-na arXiv https://doi.org/10.48550/arxiv.1907.00180	text	January 2019
A multispectral analysis of the northeastern shell of IC 443 Alarie, Alexandre; Drissen, Laurent arXiv https://doi.org/10.48550/arxiv.1908.02906	text	January 2019
Neutral iron line in the supernova remnant IC 443 and implications for MeV cosmic rays Nobukawa, Kumiko K.; Hirayama, Arisa; Shimaguchi, Aika arXiv https://doi.org/10.48550/arxiv.1908.05119	text	January 2019
Runaway O-star Bow Shocks as Particle Accelerators? The Case of AE Aur revisited Rangelov, Blagoy; Montmerle, Thierry; Federman, S. R. arXiv https://doi.org/10.48550/arxiv.1909.01424	text	January 2019
Supernova Shocks in Molecular Clouds: Velocity Distribution of Molecular Hydrogen Reach, William T.; Tram, Le Ngoc; Richter, Matthew arXiv https://doi.org/10.48550/arxiv.1909.02079	text	January 2019

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