8. teden - 22. in 23. november
Stellar Atmospheres (...continued)
- equation of radiative transfer
- vertical optical depth
- definition of gray atmospheres
- Eddington's approximation
- limb darkening
- spectral line profiles
- equivalent width
- width of spectral lines: natural, Doppler, collisions
- column density and growth curve
- using the Boltzmann and Sah equations to calculate column density
- using the Boltzmann and Sah equations to calculate column density
Literature: Carroll, Ostlie, Chap. 9
Last modified: Saturday, 15 January 2022, 12:25 AM