Space and velocity distributions of Galactic isolated old Neutron stars

Understand

I present the results of Monte-Carlo orbital simulations of Galactic Neutron Stars (NSs).

• The simulations take into account the up-to-date observed NS space and velocity distributions at birth, and account for their formation rate.
• I simulate two populations of NSs.
• Objects in the first population were born in the Galactic disk at a constant rate, in the past 12 Gyr.