Suzaku observation of TeV J2032+4130

Details Suzaku observation of TeV J2032+4130 Suzaku observation of TeV J2032+4130

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248...41m&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

Particle Accelerators, Star Formation, Stellar Atmospheres, X-Ray Sources (Astronomical), Particle Acceleration, Star Formation, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, X-Ray Sources, X-Ray Bursts

Scientific paper

TeV J2032+4130 is the first unidentified TeV γ-ray source discovered by HEGRA. The position is coincident with OB association Cyg OB2. Recently, the Fermi Gamma-ray Space Telescope discovered a γ-ray pulsar in this field. Subsequent radio observation also detected the pulsation, and determined the accurate position. The TeV γ-ray emission would be originated by the pulsar wind nebula. We observed TeV J2032+4130 with Suzaku for about 40 ksec. We discovered diffuse X-ray emission at the position of the γ-ray pulsar.

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