F8250p Structure and Evolution of Stars

Faculty of Science
Spring 2000
Extent and Intensity
2/0/0. Type of Completion: zk (examination).
Teacher(s)
doc. RNDr. Vladimír Štefl, CSc. (lecturer)
Guaranteed by
prof. RNDr. Michal Lenc, Ph.D.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: doc. RNDr. Vladimír Štefl, CSc.
Prerequisites
Knowledges on the level of course of theoretical physics, above all quatum and statistical physics and thermodynamics
Course Enrolment Limitations
The course is also offered to the students of the fields other than those the course is directly associated with.
fields of study / plans the course is directly associated with
Syllabus
  • 1. Methods obtaining of spectra 2. Spectra of atoms and molecules in astrophysics 3. Profils of spectral lines, broadening and shift lines 4. Radiative tranfer equation and their solution 5. Curves of growth, determination of chemical composition of atmospheres 6. Models of atmospheres, grey atmospheres, LTE, NLTE
Literature
  • BÖHM-VITENSE, Erika. Introduction to stellar astrophysics. Vol. 2, Stellar atmosphere. 1st pub. Cambridge: Cambridge University Press, 1997, xi, 249 s. ISBN 0-521-34403-4. info
  • Mihalas, D.: Stellar atmospheres. Freeman & Co., San Francisco, 1978.
  • Rutten, R.J.: Radiative transfer in stellar atmospheres.http://www.astro.uu.nl/~rutten
Language of instruction
Czech
Further Comments
The course is taught annually.
The course is taught: every week.
  • Enrolment Statistics (recent)
  • Permalink: https://is.muni.cz/course/sci/spring2000/F8250p