Published January 10, 2012 | Version v1
Journal article

CONSTRAINING RADIO EMISSION FROM MAGNETARS

  • 1. Department of Physics, Rutherford Physics Building, McGill University, 3600 University Street, Montreal, Quebec H3A 2T8 (Canada)
  • 2. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn (Germany)
  • 3. Netherlands Institute for Radio Astronomy (ASTRON), Postbus 2, 7990 AA Dwingeloo (Netherlands)

Description

We report on radio observations of five magnetars and two magnetar candidates carried out at 1950 MHz with the Green Bank Telescope in 2006-2007. The data from these observations were searched for periodic emission and bright single pulses. Also, monitoring observations of magnetar 4U 0142+61 following its 2006 X-ray bursts were obtained. No radio emission was detected for any of our targets. The non-detections allow us to place luminosity upper limits of L1950 ∼< 1.60 mJy kpc2 for periodic emission and L1950,single ∼< 7.6 Jy kpc2 for single pulse emission. These are the most stringent limits yet for the magnetars observed. The resulting luminosity upper limits together with previous results are discussed, as is the importance of further radio observations of radio-loud and radio-quiet magnetars.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/744/2/97

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
744
Journal Issue
2
Journal Page Range
[9 p.]
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43094393
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
EMISSION; LUMINOSITY; PERIODICITY; PULSARS; STARS; TELESCOPES
Descriptors DEC
COSMIC RADIO SOURCES; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; VARIATIONS