PSR J2021+4026 in the Gamma Cygni Region: The First Variable y-Ray Pulsar Seen by the Fermi Lat
dc.citation.issueNumber | L2 | en_US |
dc.citation.journalTitle | The Astrophysical Journal Letters | en_US |
dc.citation.volumeNumber | 777 | en_US |
dc.contributor.author | Baring, M.G. | en_US |
dc.contributor.author | Allafort, A. | en_US |
dc.contributor.author | Baldini, L. | en_US |
dc.contributor.author | Ballet, J. | en_US |
dc.contributor.author | Barbiellini, G. | en_US |
dc.contributor.author | Bastieri, D. | en_US |
dc.contributor.author | Bellazzini, R. | en_US |
dc.contributor.author | Bonamente, E. | en_US |
dc.contributor.author | Bottacini, E. | en_US |
dc.contributor.author | Brandt, T.J. | en_US |
dc.contributor.author | Bregeon, J. | en_US |
dc.contributor.author | Bruel, P. | en_US |
dc.contributor.author | Buehler, R. | en_US |
dc.contributor.author | Buson, S. | en_US |
dc.contributor.author | Caliandro, G.A. | en_US |
dc.contributor.author | Cameron, R.A. | en_US |
dc.contributor.author | Caraveo, P.A. | en_US |
dc.contributor.author | Cecchi, C. | en_US |
dc.contributor.author | Chaves, R.C.G. | en_US |
dc.contributor.author | Chekhtman, A. | en_US |
dc.contributor.author | Chiang, J. | en_US |
dc.contributor.author | Chiaro, G. | en_US |
dc.contributor.author | Ciprini, S. | en_US |
dc.contributor.author | Claus, R. | en_US |
dc.contributor.author | D'Ammando, F. | en_US |
dc.contributor.author | de Palma, F. | en_US |
dc.contributor.author | Digel, S.W. | en_US |
dc.contributor.author | Di Venere, L. | en_US |
dc.contributor.author | Drell, P.S. | en_US |
dc.contributor.author | Favuzzi, C. | en_US |
dc.contributor.author | Ferrara, E.C. | en_US |
dc.contributor.author | Franckowiak, A. | en_US |
dc.contributor.author | Fusco, P. | en_US |
dc.contributor.author | Gargano, F. | en_US |
dc.contributor.author | Gasparrini, D. | en_US |
dc.contributor.author | Giglietto, N. | en_US |
dc.contributor.author | Giroletti, M. | en_US |
dc.contributor.author | Glanzman, T. | en_US |
dc.contributor.author | Godfrey, G. | en_US |
dc.contributor.author | Grenier, I.A. | en_US |
dc.contributor.author | Guiriec, S. | en_US |
dc.contributor.author | Hadasch, D. | en_US |
dc.contributor.author | Harding, A.K. | en_US |
dc.contributor.author | Hayashida, M. | en_US |
dc.contributor.author | Hayashi, K. | en_US |
dc.contributor.author | Hays, E. | en_US |
dc.contributor.author | Hewitt, J. | en_US |
dc.contributor.author | Hill, A.B. | en_US |
dc.contributor.author | Horan, D. | en_US |
dc.contributor.author | Hou, X. | en_US |
dc.contributor.author | Jogler, T. | en_US |
dc.contributor.author | Johnson, A.S. | en_US |
dc.contributor.author | Johnson, T.J. | en_US |
dc.contributor.author | Kerr, M. | en_US |
dc.contributor.author | Knödlseder, J. | en_US |
dc.contributor.author | Kuss, M. | en_US |
dc.contributor.author | Lande, J. | en_US |
dc.contributor.author | Larsson, S. | en_US |
dc.contributor.author | Latronico, L. | en_US |
dc.contributor.author | Lemoine-Goumard, M. | en_US |
dc.contributor.author | Lande, J. | en_US |
dc.contributor.author | Loparco, F. | en_US |
dc.contributor.author | Lubrano, P. | en_US |
dc.contributor.author | Malyshev, D. | en_US |
dc.contributor.author | Marelli, M. | en_US |
dc.contributor.author | Mayer, M. | en_US |
dc.contributor.author | Mazziotta, M.N. | en_US |
dc.contributor.author | Mehault, J. | en_US |
dc.contributor.author | Mizuno, T. | en_US |
dc.contributor.author | Monzani, M.E. | en_US |
dc.contributor.author | Morselli, A. | en_US |
dc.contributor.author | Murgia, S. | en_US |
dc.contributor.author | Nemmen, R. | en_US |
dc.contributor.author | Nuss, E. | en_US |
dc.contributor.author | Ohsugi, T. | en_US |
dc.contributor.author | Omodei, N. | en_US |
dc.contributor.author | Orienti, M. | en_US |
dc.contributor.author | Orlando, E. | en_US |
dc.contributor.author | Paneque, D. | en_US |
dc.contributor.author | Pesce-Rollins, M. | en_US |
dc.contributor.author | Pierbattista, M. | en_US |
dc.contributor.author | Piron, F. | en_US |
dc.contributor.author | Pivato, G. | en_US |
dc.contributor.author | Porter, T.A. | en_US |
dc.contributor.author | Rainò, S. | en_US |
dc.contributor.author | Rando, R. | en_US |
dc.contributor.author | Ray, P.S. | en_US |
dc.contributor.author | Razzano, M. | en_US |
dc.contributor.author | Reimer, O. | en_US |
dc.contributor.author | Reposeur, T. | en_US |
dc.contributor.author | Romani, R.W. | en_US |
dc.contributor.author | Sartori, A. | en_US |
dc.contributor.author | Saz Parkinson, P.M. | en_US |
dc.contributor.author | Sgrò, C. | en_US |
dc.contributor.author | Siskind, E.J. | en_US |
dc.contributor.author | Smith, D.A. | en_US |
dc.contributor.author | Spinelli, P. | en_US |
dc.contributor.author | Strong, A.W. | en_US |
dc.contributor.author | Takahashi, H. | en_US |
dc.contributor.author | Thayer, J.B. | en_US |
dc.contributor.author | Thompson, D.J. | en_US |
dc.contributor.author | Tibaldo, L. | en_US |
dc.contributor.author | Tinivella, M. | en_US |
dc.contributor.author | Torres, D.F. | en_US |
dc.contributor.author | Tosti, G. | en_US |
dc.contributor.author | Uchiyama, Y. | en_US |
dc.contributor.author | Usher, T.L. | en_US |
dc.contributor.author | Vandenbroucke, J. | en_US |
dc.contributor.author | Vasileiou, V. | en_US |
dc.contributor.author | Venter, C. | en_US |
dc.contributor.author | Vianello, G. | en_US |
dc.contributor.author | Vitale, V. | en_US |
dc.contributor.author | Winer, B.L. | en_US |
dc.contributor.author | Wood, K.S. | en_US |
dc.date.accessioned | 2013-10-18T17:28:13Z | en_US |
dc.date.available | 2014-04-19T05:10:04Z | en_US |
dc.date.issued | 2013 | en_US |
dc.description.abstract | Long-term monitoring of PSR J2021+4026 in the heart of the Cygnus region with the Fermi Large Area Telescope unveiled a sudden decrease in flux above 100 MeV over a timescale shorter than a week. The "jump" was near MJD 55850 (2011 October 16), with the flux decreasing from (8.33 ± 0.08) × 10–10 erg cm–2 s–1 to (6.86 ± 0.13) × 10–10 erg cm–2 s–1. Simultaneously, the frequency spindown rate increased from (7.8 ± 0.1) × 10–13 Hz s–1 to (8.1 ± 0.1) × 10–13 Hz s–1. Significant (>5σ) changes in the pulse profile and marginal (<3σ) changes in the emission spectrum occurred at the same time. There is also evidence for a small, steady flux increase over the 3 yr preceding MJD 55850. This is the first observation at γ-ray energies of mode changes and intermittent behavior, observed at radio wavelengths for other pulsars. We argue that the change in pulsed γ-ray emission is due to a change in emission beaming and we speculate that it is precipitated by a shift in the magnetic field structure, leading to a change of either effective magnetic inclination or effective current. | en_US |
dc.embargo.terms | 6 months | en_US |
dc.identifier.citation | Baring, M.G., Allafort, A., Baldini, L., et al.. "PSR J2021+4026 in the Gamma Cygni Region: The First Variable y-Ray Pulsar Seen by the Fermi Lat." <i>The Astrophysical Journal Letters,</i> 777, no. L2 (2013) The American Astronomical Society: http://dx.doi.org/10.1088/2041-8205/777/1/L2. | en_US |
dc.identifier.doi | http://dx.doi.org/10.1088/2041-8205/777/1/L2 | en_US |
dc.identifier.uri | https://hdl.handle.net/1911/72217 | en_US |
dc.language.iso | eng | en_US |
dc.publisher | The American Astronomical Society | en_US |
dc.rights | Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. | en_US |
dc.subject.keyword | gamma rays | en_US |
dc.subject.keyword | stars – pulsars | en_US |
dc.subject.keyword | individual (PSR J2021+4026) – stars | en_US |
dc.subject.keyword | neutron | en_US |
dc.title | PSR J2021+4026 in the Gamma Cygni Region: The First Variable y-Ray Pulsar Seen by the Fermi Lat | en_US |
dc.type | Journal article | en_US |
dc.type.dcmi | Text | en_US |
dc.type.publication | publisher version | en_US |