Pulsar#
- class gammapy.astro.source.Pulsar(P_0='0.1 s', B='1e10 G', n=3, I=<Quantity 1.e+45 cm2 g>, R=<Quantity 1000000. cm>, age=None, L_0=None)#
Bases:
object
Magnetic dipole spin-down pulsar model.
- Parameters
- P_0float
Period at birth
- B
Quantity
Magnetic field strength at the poles (Gauss)
- nfloat
Spin-down braking index
- Ifloat
Moment of inertia
- Rfloat
Radius
Methods Summary
energy_integrated
(t)Total energy released by a given time.
luminosity_spindown
(t)Spin down luminosity.
magnetic_field
(t)Magnetic field at polar cap (assumed constant).
period
(t)Rotation period.
period_dot
(t)Period derivative at age t.
tau
(t)Characteristic age at real age t.
Methods Documentation