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Enhanced x-ray emission coinciding with giant radio pulses from the Crab Pulsar.
Enoto, Teruaki; Terasawa, Toshio; Kisaka, Shota; Hu, Chin-Ping; Guillot, Sebastien; Lewandowska, Natalia; Malacaria, Christian; Ray, Paul S; Ho, Wynn C G; Harding, Alice K; Okajima, Takashi; Arzoumanian, Zaven; Gendreau, Keith C; Wadiasingh, Zorawar; Markwardt, Craig B; Soong, Yang; Kenyon, Steve; Bogdanov, Slavko; Majid, Walid A; Güver, Tolga; Jaisawal, Gaurava K; Foster, Rick; Murata, Yasuhiro; Takeuchi, Hiroshi; Takefuji, Kazuhiro; Sekido, Mamoru; Yonekura, Yoshinori; Misawa, Hiroaki; Tsuchiya, Fuminori; Aoki, Takahiko; Tokumaru, Munetoshi; Honma, Mareki; Kameya, Osamu; Oyama, Tomoaki; Asano, Katsuaki; Shibata, Shinpei; Tanaka, Shuta J.
Afiliação
  • Enoto T; Cluster for Pioneering Research, RIKEN, Wako 351-0198, Japan. teruaki.enoto@riken.jp terasawa@icrr.u-tokyo.ac.jp kisaka@hiroshima-u.ac.jp cphu0821@cc.ncue.edu.tw.
  • Terasawa T; Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan. teruaki.enoto@riken.jp terasawa@icrr.u-tokyo.ac.jp kisaka@hiroshima-u.ac.jp cphu0821@cc.ncue.edu.tw.
  • Kisaka S; Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, Mitaka 181-8588, Japan.
  • Hu CP; Interdisciplinary Theoretical Science Research Group, RIKEN, Wako 351-0198, Japan.
  • Guillot S; Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Sendai 980-8578, Japan. teruaki.enoto@riken.jp terasawa@icrr.u-tokyo.ac.jp kisaka@hiroshima-u.ac.jp cphu0821@cc.ncue.edu.tw.
  • Lewandowska N; Astronomical Institute, Tohoku University, Sendai 980-8578, Japan.
  • Malacaria C; Department of Physical Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan.
  • Ray PS; Cluster for Pioneering Research, RIKEN, Wako 351-0198, Japan. teruaki.enoto@riken.jp terasawa@icrr.u-tokyo.ac.jp kisaka@hiroshima-u.ac.jp cphu0821@cc.ncue.edu.tw.
  • Ho WCG; Department of Physics, National Changhua University of Education, Changhua 50007, Taiwan.
  • Harding AK; Department of Astronomy, Kyoto University, Kyoto 606-8502, Japan.
  • Okajima T; Institut de Recherche en Astrophysique, Toulouse 31028, France.
  • Arzoumanian Z; Department of Physics and Astronomy, Haverford College, Haverford, PA 19041, USA.
  • Gendreau KC; NASA Marshall Space Flight Center, National Space Science and Technology Center, Huntsville, AL 35805, USA.
  • Wadiasingh Z; Universities Space Research Association, Science and Technology Institute, Huntsville, AL 35805, USA.
  • Markwardt CB; US Naval Research Laboratory, Washington, DC 20375, USA.
  • Soong Y; Department of Physics and Astronomy, Haverford College, Haverford, PA 19041, USA.
  • Kenyon S; Mathematical Sciences and STAG Research Centre, University of Southampton, Southampton SO17 1BJ, UK.
  • Bogdanov S; NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
  • Majid WA; Theoretical Division, Los Alamos National Laboratory, Los Alamos, NM 87545, USA.
  • Güver T; NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
  • Jaisawal GK; NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
  • Foster R; NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
  • Murata Y; NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
  • Takeuchi H; Universities Space Research Association, Columbia, MD 21046, USA.
  • Takefuji K; NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
  • Sekido M; NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
  • Yonekura Y; NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
  • Misawa H; Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA.
  • Tsuchiya F; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
  • Aoki T; California Institute of Technology, Pasadena, CA 91125, USA.
  • Tokumaru M; Istanbul University, Science Faculty, Department of Astronomy and Space Sciences, Beyazit, 34119 Istanbul, Turkey.
  • Honma M; National Space Institute, Technical University of Denmark, Elektrovej 327-328, Denmark.
  • Kameya O; Massachusetts Institute of Technology Kavli Institute for Astrophysics and Space Research, Cambridge, MA 02139, USA.
  • Oyama T; Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.
  • Asano K; Usuda Deep Space Center, Japan Aerospace Exploration Agency, Saku 384-0306, Japan.
  • Shibata S; Department of Space and Astronautical Science, SOKENDAI (The Graduate University for Advanced Studies), Sagamihara 252-5210, Japan.
  • Tanaka SJ; Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.
Science ; 372(6538): 187-190, 2021 04 09.
Article em En | MEDLINE | ID: mdl-33833123
ABSTRACT
Giant radio pulses (GRPs) are sporadic bursts emitted by some pulsars that last a few microseconds and are hundreds to thousands of times brighter than regular pulses from these sources. The only GRP-associated emission outside of radio wavelengths is from the Crab Pulsar, where optical emission is enhanced by a few percentage points during GRPs. We observed the Crab Pulsar simultaneously at x-ray and radio wavelengths, finding enhancement of the x-ray emission by 3.8 ± 0.7% (a 5.4σ detection) coinciding with GRPs. This implies that the total emitted energy from GRPs is tens to hundreds of times higher than previously known. We discuss the implications for the pulsar emission mechanism and extragalactic fast radio bursts.
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Texto completo: 1 Base de dados: MEDLINE Idioma: En Revista: Science Ano de publicação: 2021 Tipo de documento: Article
Texto completo
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Texto completo: 1 Base de dados: MEDLINE Idioma: En Revista: Science Ano de publicação: 2021 Tipo de documento: Article