Searching for X-ray counterparts of fermi gamma-ray pulsars in suzaku observations

Yu Aoki, Takahiro Enomoto, Yoichi Yatsu, Nobuyuki Kawai, Takeshi Nakamori, Jun Kataoka, P. Saz Parkinson

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Citation (Scopus)

Abstract

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.

Original languageEnglish
Title of host publicationDeath of Massive Stars
Subtitle of host publicationSupernovae and Gamma-Ray Bursts
EditorsPeter W. A. San Antonio, Nobuyuki Kawai, Elena Pian
Pages317-318
Number of pages2
EditionS279
DOIs
Publication statusPublished - 2011 Apr 1

Publication series

NameProceedings of the International Astronomical Union
NumberS279
Volume7
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

    Fingerprint

Keywords

  • Gamma-ray pulsars. Fermi.
  • Pulsar
  • 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

Cite this

Aoki, Y., Enomoto, T., Yatsu, Y., Kawai, N., Nakamori, T., Kataoka, J., & Saz Parkinson, P. (2011). Searching for X-ray counterparts of fermi gamma-ray pulsars in suzaku observations. In P. W. A. San Antonio, N. Kawai, & E. Pian (Eds.), Death of Massive Stars: Supernovae and Gamma-Ray Bursts (S279 ed., pp. 317-318). (Proceedings of the International Astronomical Union; Vol. 7, No. S279). https://doi.org/10.1017/S1743921312013130