Radiative Transfer in Stellar Atmospheres

Date: 30 April 2011, 09:08

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This is the current version of lecture notes for the Utrecht third-year astronomy course
on stellar atmospheres. The main topic treated in this 30-hour course is the classical
theory of radiative transfer for explaining stellar spectra. The reason to emphasize this
topic over the many newer subjects of astrophysical interest oered by stellar atmospheres is that it needs relatively much attention to be mastered. Radiative transfer in gaseous media that are neither optically thin nor completely opaque is a key part of astrophysics, but it is not a transparent subject.
This course requires familiarity with the basic quantities and processes of radiative transfer. At Utrecht I treat these in a more basic course that follows the first chapter of
Rybicki and Lightman (1979) and is summarized in Chapter 2 here. The present lecture notes are roughly a middle road between Mihalas (1970) and the books by Novotny (1973) and B?ohm-Vitense (1989), at about the level of Gray (1992) but emphasizing radiative transfer rather than observational techniques and data interpretation.

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