Astrophysics and Space Science

, Volume 308, Issue 1, pp 95–99

Chandra smells a RRAT

X-ray detection of a rotating radio transient

Authors

    • Harvard-Smithsonian Center for Astrophysics
  • Maura McLaughlin
    • University of West Virginia
  • Stephen Reynolds
    • North Carolina State University
  • Kazik Borkowski
    • North Carolina State University
  • Nanda Rea
    • SRON Netherlands Institute for Space Research
  • Andrea Possenti
    • Osservatorio Astronomico di Cagliari
  • Gianluca Israel
    • Osservatorio Astronomico di Roma
  • Marta Burgay
    • Osservatorio Astronomico di Cagliari
  • Fernando Camilo
    • Columbia University
  • Shami Chatterjee
    • Harvard-Smithsonian Center for Astrophysics
  • Michael Kramer
    • Jodrell Bank Observatory
  • Andrew Lyne
    • Jodrell Bank Observatory
  • Ingrid Stairs
    • University of British Columbia
Original Article

DOI: 10.1007/s10509-007-9352-8

Cite this article as:
Gaensler, B.M., McLaughlin, M., Reynolds, S. et al. Astrophys Space Sci (2007) 308: 95. doi:10.1007/s10509-007-9352-8

Abstract

“Rotating RAdio Transients” (RRATs) are a newly discovered astronomical phenomenon, characterised by occasional brief radio bursts, with average intervals between bursts ranging from minutes to hours. The burst spacings allow identification of periodicities, which fall in the range 0.4 to 7 seconds. The RRATs thus seem to be rotating neutron stars, albeit with properties very different from the rest of the population. We here present the serendipitous detection with the Chandra X-ray Observatory of a bright point-like X-ray source coincident with one of the RRATs. We discuss the temporal and spectral properties of this X-ray emission, consider counterparts in other wavebands, and interpret these results in the context of possible explanations for the RRAT population.

Keywords

Pulsars: individual (J1819-1458)Stars: flare, neutronX-rays: stars

PACS

97.60.Gb97.60.Jd98.70.Qy

Copyright information

© Springer Science+Business Media B.V. 2007