Astrophysical source models (gammapy.astro.source
)¶
Introduction¶
The gammapy.astro.source
module contains classes of source models, which can be used for population synthesis of galactic gamma-ray sources.
Getting Started¶
TODO: add basic example.
Using gammapy.astro.source
¶
The following source models are available:
Reference/API¶
gammapy.astro.source Package¶
Astrophysical source models.
Classes¶
PWN ([pulsar, snr, eta_e, eta_B, morphology, age]) |
Simple pulsar wind nebula (PWN) evolution model. |
Pulsar ([P_0, logB, n, I, R, age, L_0, ...]) |
Magnetic dipole spin-down pulsar model. |
SNR ([e_sn, theta, n_ISM, m_ejecta, ...]) |
Simple supernova remnant (SNR) evolution model. |
SNRTrueloveMcKee (*args, **kwargs) |
SNR model according to Truelove & McKee (1999). |
SimplePulsar (P, P_dot[, I, R]) |
Magnetic dipole spin-down model for a pulsar. |