Gamma-ray emission from pulsar/massive-star binaries
classification
🌌 astro-ph.HE
keywords
binariesgamma-raypulsaraspectsdiscussemissionenergieshigh
read the original abstract
I present a review of the main phenomenological properties at high energies related to massive gamma-ray binaries and I discuss some aspects of pulsar models for these objects.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.