The high-energy emission of millisecond pulsars. (arXiv:2004.03128v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Torres_D/0/1/0/all/0/1">Diego F. Torres</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Li_J/0/1/0/all/0/1">Jian Li</a>

This chapter provides a phenomenological appraisal of the high-energy
emission of millisecond pulsars. We comment on some of their properties as a
population, as well as consider the especial cases of transitional pulsars,
other redbacks, and black widow systems.

This chapter provides a phenomenological appraisal of the high-energy
emission of millisecond pulsars. We comment on some of their properties as a
population, as well as consider the especial cases of transitional pulsars,
other redbacks, and black widow systems.

http://arxiv.org/icons/sfx.gif