Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2010-01-11
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
11 pages, 4 figures
Scientific paper
The rising cosmic ray positron fraction reported by the PAMELA collaboration has lead to a great deal of interest in astrophysical sources of energetic electrons and positrons, including pulsars. In this paper, we calculate the spectrum of synchrotron emission from electrons and positrons injected from 376 young pulsars (<10^6 years) contained in the ATNF catalog, and compare our results to observations. We find that if objects such as the Vela and Crab pulsars have injected ~10^48 erg or more in energetic electrons and/or positrons, they are expected to produce bright and distinctive features in the synchrotron sky. Intriguingly, we predict hard synchrotron emission from these regions of the sky which is qualitatively similar to that observed by WMAP.
Hooper Dan
Kelso Christopher M.
No associations
LandOfFree
Synchrotron Emission From Young And Nearby 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 Synchrotron Emission From Young And Nearby Pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Synchrotron Emission From Young And Nearby Pulsars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-458591