Abstract
PSRs J0248+6021 & J2240+5832 are “typical” young, radio-loud pulsars detected in GeV gamma rays using the Large Area Telescope (LAT) on the Fermi satellite. “Typical” because their P, P lie mid-range of those of the new gamma-ray pulsars, but also because of some nagging little observational problems. This paper focusses on the observables available to help interpret the wave of new gamma-ray pulsar findings, and some of their limitations.
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© 2011 Springer-Verlag Berlin Heidelberg
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Smith, D.A., Fermi LAT Collaboration. (2011). “Garden-variety” Gamma-ray Pulsars J0248+6021 & J2240+5832. In: Torres, D., Rea, N. (eds) High-Energy Emission from Pulsars and their Systems. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-17251-9_5
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DOI: https://doi.org/10.1007/978-3-642-17251-9_5
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