The many faces of pulsars

Pulsars are rapidly rotating, strongly magnetised neutron stars, 
emitting flashes of non-thermal radiation covering up to eighteen decades of 
energy in the electromagnetic spectrum.
They are powerful tools used in physics, astronomy and even cosmology.
I’ll review their observational status and prospects for the future.
I’ll then present current models of high-energy processes as well as new
theoretical developments in modeling pulsars and their wind zones.


Mercredi, 30 mai, 2018 - 14:00 to 15:00

Salle / Local: 

salle 483A

Nom/Prénom // Last name/First name: 

Bronek Rudak


Nicolaus Copernicus Astronomical Center, Warsaw

Equipe(s) organisatrice(s) / Organizing team(s): 

  • Astrophysique à Haute Energie