Observations of Galactic Pulsars and Shell-Type SNRs with the Whipple 10 m Imaging Atmospheric Cherenkov Telescope

Details Observations of Galactic Pulsars and Shell-Type SNRs with the Whipple 10 m Imaging Atmospheric Cherenkov Telescope Observations of Galactic Pulsars and Shell-Type SNRs with the Whipple 10 m Imaging Atmospheric Cherenkov Telescope

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....6.2485h&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

2

Scientific paper

Observations of pulsar systems and supernova remnants have been conducted at the Whipple Observatory using the 10 m imaging atmospheric Cherenkov telescope. Since the summer of 1999, a high resolution 490 pixel camera has been in place yielding a significant increase in detector sensitivity. We present the results of these observations and the implications they have on the various theories of very high energy emissions.

Affiliated with

Also associated with

No associations

Rating

Observations of Galactic Pulsars and Shell-Type SNRs with the Whipple 10 m Imaging Atmospheric Cherenkov Telescope does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Observations of Galactic Pulsars and Shell-Type SNRs with the Whipple 10 m Imaging Atmospheric Cherenkov Telescope, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of Galactic Pulsars and Shell-Type SNRs with the Whipple 10 m Imaging Atmospheric Cherenkov Telescope will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-796135