Pulsars in a Bubble? Following Electron Diffusion in the Galaxy with TeV Gamma Rays
by Henrike Fleischhack, A. Albert, C. Alvarez, R. Arceo, H. A. Ayala Solares, J. F. Beacom, R. Bird, C. A. Brisbois, K. S. Caballero-Mora, A. Carraminana, S. Casanova, P. Cristofari, P. Coppi, B. L. Dingus, M. A. DuVernois, K. L. Engel, J. A. Goodman, T. Greenshaw, J. P. Harding, B. Hona, P. H. Huentemeyer, H. Li, T. Linden, K. Malone, J. Martinez-Castro, M. A. Mostafa, M. U. Nisa, C. Riviere, F. Salesa Greus, A. Sandoval, A. J. Smith, W. Springer, T. Sudoh, K. Tollefson, A. Zepeda, and H. Zhou
Published onMay 31, 2019
Pulsars in a Bubble? Following Electron Diffusion in the Galaxy with TeV Gamma Rays
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Abstract
TeV Halos, extended regions of gamma-ray emission around pulsars, are a new class of gamma-ray sources. They can be used to study pulsar properties and e+/e- diffusion on scales of ~10 pc, as well as to find misaligned pulsars. We outline the contributions of future gamma-ray instruments to the study of TeV Halos and the expected physics outcomes.
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