We report the Suzaku follow-up observations of the Gamma-ray pulsars, 1FGL J0614,13328, J1044.55737, J1741.82101, and J1813.31246, which were discovered by the Fermi Gamma-ray observatory. Analysing Suzaku/XIS data, we detected X-ray counterparts of these pulsars in the Fermi error circle and interpreted their spectra with absorbed power-law functions. These results indicate that the origin of these X-ray sources is non-thermal emission from the pulsars or from Pulsar Wind Nebulae (PWNe) surrounding them. Moreover we found that J1741.82101 exhibits a peculiar profile: spin-down luminosity vs flux ratio between X-and gamma-rays is unusually large compared to usual radio pulsars.
|Title of host publication||Death of Massive Stars|
|Subtitle of host publication||Supernovae and Gamma-Ray Bursts|
|Editors||Peter W. A. San Antonio, Nobuyuki Kawai, Elena Pian|
|Number of pages||2|
|Publication status||Published - 2011 Apr 1|
|Name||Proceedings of the International Astronomical Union|
- Gamma-ray pulsars. Fermi.
- Pulsar wind nebulae
ASJC Scopus subject areas
- Medicine (miscellaneous)
- Astronomy and Astrophysics
- Nutrition and Dietetics
- Public Health, Environmental and Occupational Health
- Space and Planetary Science