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The fermi gamma-ray space telescope discovers the pulsar in the young galactic supernova remnant CTA 1

  • A. A. Abdo
  • , M. Ackermann
  • , W. B. Atwood
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , M. G. Baring
  • , D. Bastieri
  • , B. M. Baughman
  • , K. Bechtol
  • , R. Bellazzini
  • , B. Berenji
  • , R. D. Blandford
  • , E. D. Bloom
  • , G. Bogaert
  • , E. Bonamente
  • , A. W. Borgland
  • , J. Bregeon
  • , A. Brez
  • , M. Brigida
  • P. Bruel, T. H. Burnett, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, P. Carlson, J. M. Casandjian, C. Cecchi, E. Charles, A. Chekhtman, C. C. Cheung, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, L. R. Cominsky, J. Conrad, S. Cutini, D. S. Davis, C. D. Dermer, A. De Angelis, F. De Palma, S. W. Digel, M. Dormody, E. Do Couto E Silva, P. S. Drell, R. Dubois, D. Dumora, Y. Edmonds, C. Farnier, W. B. Focke, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, S. Germani, B. Giebels, N. Giglietto, F. Giordano, T. Glanzman, G. Godfrey, I. A. Grenier, M. H. Grondin, J. E. Grove, L. Guillemot, S. Guiriec, A. K. Harding, R. C. Hartman, E. Hays, R. E. Hughes, G. Jóhannesson, A. S. Johnson, R. P. Johnson, T. J. Johnson, W. N. Johnson, T. Kamae, Y. Kanai, G. Kanbach, H. Katagiri, N. Kawai, M. Kerr, T. Kishishita, B. Kiziltan, J. Knödlseder, M. L. Kocian, N. Komin, F. Kuehn, M. Kuss, L. Latronico, M. Lemoine-Goumard, F. Longo, V. Lonjou, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, A. Makeev, M. Marelli, M. N. Mazziotta, J. E. McEnery, S. McGlynn, C. Meurer, P. F. Michelson, T. Mineo, W. Mitthumsiri, T. Mizuno, A. A. Moiseev, C. Monte, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, T. Nakamori, P. L. Nolan, E. Nuss, M. Ohno, T. Ohsugi, A. Okumura, N. Omodei, E. Orlando, J. F. Ormes, M. Ozaki, D. Paneque, J. H. Panetta, D. Parent, V. Pelassa, M. Pepe, M. Pesce-Rollins, G. Piano, L. Pieri, F. Piron, T. A. Porter, S. Rainò, R. Rando, P. S. Ray, M. Razzano, A. Reimer, O. Reimer, T. Reposeur, S. Ritz, L. S. Rochester, A. Y. Rodriguez, R. W. Romani, M. Roth, F. Ryde, H. F.W. Sadrozinski, D. Sanchez, A. Sander, P. M. Saz Parkinson, T. L. Schalk, A. Sellerholm, C. Sgrò, E. J. Siskind, D. A. Smith, P. D. Smith, G. Spandre, P. Spinelli, J. L. Starck, M. S. Strickman, D. J. Suson, H. Tajima, H. Takahashi, T. Takahashi, T. Tanaka, J. B. Thayer, J. G. Thayer, D. J. Thompson, S. E. Thorsett, L. Tibaldo, D. F. Torres, G. Tosti, A. Tramacere, T. L. Usher, A. Van Etten, N. Vilchez, V. Vitale, P. Wang, K. Watters, B. L. Winer, K. S. Wood, H. Yasuda, T. Ylinen, M. Ziegler
  • National Research Council
  • Naval Research Laboratory
  • Kavli Institute for Particle Astrophysics and Cosmology
  • Stanford Linear Accelerator Center
  • University of California at Santa Cruz
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • Université Paris-Diderot
  • INFN Sezione di Trieste
  • University of Trieste
  • Rice University
  • INFN
  • University of Padova
  • The Ohio State University
  • INFN Sezione di Perugia
  • University of Perugia
  • Politecnico di Bari
  • INFN Sezione di Bari
  • University of Washington
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • KTH Royal Institute of Technology
  • George Mason University
  • NASA Goddard Space Flight Center
  • Centre national de la recherche scientifique
  • Sonoma State University
  • Stockholm University
  • Science and Research Directorate
  • Biochemical and Environmental Engineering
  • and Physics University of Udine
  • Université Paris-Sud
  • Univ. Bordeaux
  • Hiroshima University
  • University of Maryland, College Park
  • Tokyo Institute of Technology
  • Max Planck Institut für Extraterrestrische Physik
  • RIKEN (The Institute of Physical and Chemical Research)
  • ISAS/JAXA
  • University of
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
  • University of Rome “Tor Vergata”
  • University of Tokyo
  • University of Denver
  • University of São Paulo
  • NYCB Real-Time Computing Inc.
  • Purdue University Northwest
  • Pompeu Fabra University (UPF)
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Kalmar

Research output: Contribution to journalArticlepeer-review

Abstract

Energetic young pulsars and expanding blast waves [supernova remnants (SNRs)] are the most visible remains after massive stars, ending their lives, explode in core-collapse supernovae. The Fermi Gamma-Ray Space Telescope has unveiled a radio quiet pulsar located near the center of the compact synchrotron nebula inside the supernova remnant CTA 1. The pulsar, discovered through its gamma-ray pulsations, has a period of 316.86 milliseconds and a period derivative of 3.614 × 10?13 seconds per second. Its characteristic age of 104 years is comparable to that estimated for the SNR. We speculate that most unidentified Galactic gamma-ray sources associated with star-forming regions and SNRs are such young pulsars.

Original languageEnglish
Pages (from-to)1218-1221
Number of pages4
JournalScience
Volume322
Issue number5905
DOIs
Publication statusPublished - 21 Nov 2008

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