Home List of Titles COMPTEL detection of pulsed gamma-ray emission from PSR B1509-58 up to at least 10MeV
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- COMPTEL detection of pulsed gamma-ray emission from PSR B1509-58 up to at least 10MeV
- Kuiper, L.; Hermsen, W.; Krijger, J. M.; Bennett, K.; Carraminana, A.; Schoenfelder, V.; Bailes, M.; Manchester, R. N.
- We report on the first firm detection of pulsed gamma-ray emission from PSR B1309-58 in the 0.75-30 MeV energy range in CGRO COMPTEL data collected over more than 6 years. The modulation significance in the 0.75-30 MeV pulse-phase distribution is 5.4σ and the lightcurve is similar to the lightcurves found earlier between 0.7 and 700 keV: a single broad asymmetric pulse reaching its maximum 038 +/- 0.03 in phase after the radio peak, compared to the offset of 0.30 found in the CGRO BATSE soft gamma-ray data, and 0.27 +/- 0.01 for RXTE (2-16keV), compatible with ASCA (0.7-2.2 keV). Analysis in narrower energy windows shows that the single broad pulse is significantly detected up to ~10MeV. Above 10MeV we do detect marginally significant (2.1σ) modulation with an indication for the broad pulse. However, imaging analysis shows the presence of a strong 5.6σ source at the position of the pulsar. To investigate this further, we have also analysed contemporaneous CGRO EGRET data (> 30MeV) collected over a nearly 4 year period. In the 30-100 Me V energy window, adjacent to the COMPTEL 10-30 MeV range, a 4.4σ source can be attributed to PSR B1509-58. Timing analysis in this energy window yields an insignificant signal of 1.1σ, but with a shape somewhat similar to that of the COMPTEL 10-30 MeV lightcurve. Combining the two pulse-phase distributions results in a suggestive double-peaked pulsed signal above the background level estimated in the spatial analyses, with one broad peak near phase 0.38 (aligned with the pulse observed at lower energies) and a second narrower peak near phase 0.85, which is absent for energies below 10 MeV. The modulation significance is, however, only 2.3σ and needs confirmation. Spectral analysis based on the excess counts in the broad pulse of the lightcurve shows that extrapolation of the OSSE power-law spectral fit with index -1.68 describes our data well up to 10 MeV. Above 10 MeV the spectrum breaks abruptly. The precise location of the break/bend between 10 and 30 MeV depends on the interpretation of the structure in the lighlcune measured by COMPTEL and EGRET above 10 MeV. Such a break in the spectrum of PSR B1509-58 bas recently been interpreted in the framework of polar cap models for the explanation of gamma-ray pulsars, as a signature of the exotic photon splitting process in the strong magnetic field of PSR B1509-58. For that interpretation our new spectrum constrains the co-latitude to ~2°, close to the "classical" radius of the polar cap. In the case of an outer-gap scenario, our spectrum requires a dominant synchrotron component.
- Publication type
- Journal article
- Research centre
- Swinburne University of Technology. Centre for Astrophysics and Supercomputing
- Astronomy and Astrophysics, Vol. 351, no. 1 (Nov 1999), pp. 119-132
- Publication year
- FOR Code(s)
- 0201 Astronomical and Space Sciences; 0305 Organic Chemistry; 0306 Physical Chemistry (Incl. Structural)
- Gamma rays; Observations; PSR B1509-58; Pulsars; Stars
- EDP Sciences
- Publisher URL
- Copyright © European Southern Observatory (ESO) 1999. The published version of the paper is reproduced here in accordance with the copyright policy of the publisher.
- Full text
- Peer reviewed