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/744/2/97Additional 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