Pulsede+Annihilation γ‐Ray Line from a Crab‐like Pulsar
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/478/i=2/a=701/pdf
Reference27 articles.
1. Observation of the Crab pulsar, PSR 0531 + 21, at 0.2-6.0 MeV with the FIGARO II experiment
2. Arons, J. 1981, in IAU Symp. 95, Pulsars, ed. W. Sieber & R. Wielebinski (Dordrecht: Reidel), 69
3. Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV
4. On the 440 keV line in the Crab Nebula pulsar
5. The proper motion of Geminga's optical counterpart
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