Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...447..807f&link_type=abstract
Astrophysical Journal v.447, p.807
Astronomy and Astrophysics
Astronomy
51
Gamma Rays: Observations, Stars: Pulsars: General
Scientific paper
More than 2 yr of observations performed by the Energetic Gamma Ray Experiment Telescope (EGRET) aboard the Compton Gamma Ray Observatory (CGRO) are examined for evidence of high-energy γ-ray emission from individual millisecond pulsars. Upper limits are placed on steady emission. In addition, for those millisecond pulsars for which an accurate timing solution is available, upper limits to pulsed γ-ray emission are established. The results are compared with predictions of current pulsar γ-ray emission models. In particular, the absence of a detection of γ-rays from the nearby millisecond pulsar PSR J0437-4715 severely constrains theories regarding γ-ray emission from millisecond pulsars.
Arzoumanian Zaven
Bailes Matthew
Bell Jon F.
Bertsch David L.
Brazier K. T. S.
No associations
LandOfFree
EGRET High-Energy gamma -Ray Pulsar Studies. II. Individual Millisecond Pulsars 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 EGRET High-Energy gamma -Ray Pulsar Studies. II. Individual Millisecond Pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and EGRET High-Energy gamma -Ray Pulsar Studies. II. Individual Millisecond Pulsars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1170297