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Fermi gamma-ray imaging of a radio galaxy.

The Fermi Gamma-ray Space Telescope has detected the gamma-ray glow emanating from the giant radio lobes of the radio galaxy Centaurus A. The resolved gamma-ray image shows the lobes clearly separated from the central active source. In contrast to all other active galaxies detected so far in high-en... Full description

Journal Title: Science (New York N.Y.), May 7, 2010, Vol.328(5979), pp.725-729
Main Author: Abdo, A A
Other Authors: Ackermann, M , Ajello, M , Atwood, W B , Baldini, L , Ballet, J , Barbiellini, G , Bastieri, D , Baughman, B M , Bechtol, K , Bellazzini, R , Berenji, B , Blandford, R D , Bloom, E D , Bonamente, E , Borgland, A W , Bregeon, J , Brez, A , Brigida, M , Bruel
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: E-ISSN: 1095-9203 ; DOI: 10.1126/science.1184656
Link: http://search.proquest.com/docview/733533987/?pq-origsite=primo
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title: Fermi gamma-ray imaging of a radio galaxy.
format: Article
creator:
  • Abdo, A A
  • Ackermann, M
  • Ajello, M
  • Atwood, W B
  • Baldini, L
  • Ballet, J
  • Barbiellini, G
  • Bastieri, D
  • Baughman, B M
  • Bechtol, K
  • Bellazzini, R
  • Berenji, B
  • Blandford, R D
  • Bloom, E D
  • Bonamente, E
  • Borgland, A W
  • Bregeon, J
  • Brez, A
  • Brigida, M
  • Bruel
subjects:
  • Astrophysics - High Energy Astrophysical Phenomena
  • Astrophysics - Cosmology And Extragalactic Astrophysics
ispartof: Science (New York, N.Y.), May 7, 2010, Vol.328(5979), pp.725-729
description: The Fermi Gamma-ray Space Telescope has detected the gamma-ray glow emanating from the giant radio lobes of the radio galaxy Centaurus A. The resolved gamma-ray image shows the lobes clearly separated from the central active source. In contrast to all other active galaxies detected so far in high-energy gamma-rays, the lobe flux constitutes a considerable portion (>1/2) of the total source emission. The gamma-ray emission from the lobes is interpreted as inverse Compton scattered relic radiation from the cosmic microwave background (CMB), with additional contribution at higher energies from the infrared-to-optical extragalactic background light (EBL). These measurements provide gamma-ray constraints on the magnetic field and particle energy content in radio galaxy lobes, and a promising method to probe the cosmic relic photon fields. Comment: 27 pages, includes Supplementary Online Material; corresponding authors: C.C. Cheung, Y. Fukazawa, J. Knodlseder, L. Stawarz
language: eng
source:
identifier: E-ISSN: 1095-9203 ; DOI: 10.1126/science.1184656
fulltext: no_fulltext
issn:
  • 10959203
  • 1095-9203
url: Link


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titleFermi gamma-ray imaging of a radio galaxy.
creatorAbdo, A A ; Ackermann, M ; Ajello, M ; Atwood, W B ; Baldini, L ; Ballet, J ; Barbiellini, G ; Bastieri, D ; Baughman, B M ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Blandford, R D ; Bloom, E D ; Bonamente, E ; Borgland, A W ; Bregeon, J ; Brez, A ; Brigida, M ; Bruel
contributorAbdo, A A (correspondence author) ; Abdo, A A (record owner)
ispartofScience (New York, N.Y.), May 7, 2010, Vol.328(5979), pp.725-729
identifierE-ISSN: 1095-9203 ; DOI: 10.1126/science.1184656
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subjectAstrophysics - High Energy Astrophysical Phenomena ; Astrophysics - Cosmology And Extragalactic Astrophysics;
descriptionThe Fermi Gamma-ray Space Telescope has detected the gamma-ray glow emanating from the giant radio lobes of the radio galaxy Centaurus A. The resolved gamma-ray image shows the lobes clearly separated from the central active source. In contrast to all other active galaxies detected so far in high-energy gamma-rays, the lobe flux constitutes a considerable portion (>1/2) of the total source emission. The gamma-ray emission from the lobes is interpreted as inverse Compton scattered relic radiation from the cosmic microwave background (CMB), with additional contribution at higher energies from the infrared-to-optical extragalactic background light (EBL). These measurements provide gamma-ray constraints on the magnetic field and particle energy content in radio galaxy lobes, and a promising method to probe the cosmic relic photon fields. Comment: 27 pages, includes Supplementary Online Material; corresponding authors: C.C. Cheung, Y. Fukazawa, J. Knodlseder, L. Stawarz
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atitleFermi gamma-ray imaging of a radio galaxy.
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date2010-05-07