Abstract
The 2nd Fermi-LAT pulsar catalog includes 117 γ-ray pulsars, of which roughly one third are millisecond pulsars (MSPs) while the remaining two thirds split evenly into young radio-loud and radio-quiet pulsars. Although this large population will enable future, detailed studies of emission mechanisms and the evolution of the underlying neutron star population, some nearly-universal properties are already clear and unequivocal. We discuss some of these aspects below, including the altitude of the γ-ray emission site, the shape of the γ-ray spectrum, and the implications of the latter for the radiation mechanism. © 2013 International Astronomical Union.
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Kerr, M. (2012). Pulsars in gamma rays: What Fermi is teaching us. In Proceedings of the International Astronomical Union (Vol. 8, pp. 307–312). Cambridge University Press. https://doi.org/10.1017/S1743921312023940
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