astrophysical model
C26274
concept
An astrophysical model is a theoretical or computational framework that describes and predicts the physical processes, structures, and evolution of astronomical objects and phenomena in the universe.
Observed surface forms (12)
- initial mass function ×3
- astrophysical approximation ×2
- stellar population model ×2
- astrophysical accretion model ×1
- astrophysics concept ×1
- result in astrophysics ×1
- solar physics model ×1
- solar wind model ×1
- stellar atmosphere model ×1
- stellar structure model ×1
- surface brightness profile model ×1
- theoretical astrophysics model ×1
Instances (17)
- Bondi accretion theory via concept surface "astrophysical accretion model"
- Einasto profile
- Einasto density profile
- Salpeter initial mass function via concept surface "initial mass function"
- Saha ionization equation via concept surface "astrophysics concept"
- Parker spiral model of the interplanetary magnetic field via concept surface "solar wind model"
- virial theorem via concept surface "result in astrophysics"
- Eddington standard model of stars via concept surface "stellar structure model"
- Maclaurin spheroid
- Roche–Riemann ellipsoids
- Paczynski–Wiita potential via concept surface "astrophysical approximation"
- Milne–Eddington approximation via concept surface "astrophysical approximation"
- Burkert profile
- Sérsic profile via concept surface "surface brightness profile model"
- Chabrier initial mass function via concept surface "initial mass function"
- Kroupa initial mass function via concept surface "initial mass function"
- Parker solar wind model