SUZAKU OBSERVATION OF THE NEW SOFT GAMMA REPEATER SGR 0501+4516 IN OUTBURST
Creators
- 1. Department of Physics, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)
- 2. Cosmic Radiation Laboratory, Institute of Physical and Chemical Research (RIKEN), Wako, Saitama 351-0198 (Japan)
- 3. Astronomical Institute 'Anton Pannekoek', University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam (Netherlands)
- 4. INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica - Milano, via E. Bassini 15, 20133 Milano (Italy)
- 5. CEA Saclay, DSM/Irfu/Service d'Astrophysique, Orme des Merisiers, Bat. 709, 91191 Gif sur Yvette (France)
- 6. Space Sciences Laboratory, 7 Gauss Way, University of California, Berkeley, CA 94720-7450 (United States)
- 7. INAF-Astronomical Observatory of Rome, via Frascati 33, 00040 Monteporzio Catone (RM) (Italy)
- 8. Institute of Space and Astronautical Science, JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510 (Japan)
- 9. Department of Physics, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima-ku, Tokyo 171-8501 (Japan)
- 10. NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
- 11. University of Padua, Department of Physics, via Marzolo 8, 35131 Padova (Italy)
- 12. Department of Physics and Mathematics, Aoyama Gakuin University, Sagamihara, Kanagawa 229-8558 (Japan)
- 13. MSSL, University College London, Holmbury St. Mary, Dorking RH5 6NT (United Kingdom)
Description
We present the first Suzaku observation of the new Soft Gamma Repeater, SGR 0501+4516, performed on 2008 August 26, four days after the onset of bursting activity of this new member of the magnetar family. The soft X-ray persistent emission was detected with the X-ray Imaging Spectrometer (XIS) at a 0.5-10 keV flux of 3.8 x 10-11 erg s-1cm-2, with a spectrum well fitted by an absorbed blackbody plus power-law model. The source pulsation was confirmed at a period of 5.762072 ± 0.000002 s, and 32 X-ray bursts were detected by the XIS, four of which were also detected at higher energies by the Hard X-ray Detector (HXD). The strongest burst, which occurred at 03:16:16.9 (UTC), was so bright that it caused instrumental saturation, but its precursor phase, lasting for about 200 ms, was detected successfully over the 0.5-200 keV range, with a fluence of ∼2.1 x 10-7 erg cm-2 and a peak intensity of about 89 crab. The entire burst fluence is estimated to be ∼50 times higher. The precursor spectrum was very hard, and well modeled by a combination of two blackbodies. We discuss the bursting activity and X/γ-ray properties of this newly discovered Soft Gamma Repeater in comparison with other members of the class.
Availability note (English)
Available from http://dx.doi.org/10.1088/0004-637X/693/2/L122Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal (Online)
- Journal Volume
- 693
- Journal Issue
- 2
- Journal Page Range
- p. L122-L126
- ISSN
- 1538-4357
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41029715
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- EMISSION; GAMMA RADIATION; HARD X RADIATION; MAGNETIC FIELDS; PULSARS; PULSATIONS; SOFT X RADIATION; SPECTRA; SPECTROMETERS; STARS
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; MEASURING INSTRUMENTS; RADIATIONS; X RADIATION