F8250c Structure and Evolution of Stars, ex.

Faculty of Science
Spring 2000
Extent and Intensity
0/1/0. Type of Completion: z (credit).
Teacher(s)
doc. RNDr. Vladimír Štefl, CSc. (seminar tutor)
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 of optics, atom physics, quantum a statistical physics
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. Radiation of stars 2. Spectra atoms and molecules in astrophysics 3. Shifts and broadening of spectral lines, width lines 4. Boltzmann
  • s and Saha's equations 5. Physical conditions in atmospheres 6. Radiative transfer equation, their solution and consequence
Literature
  • Bowers, R. L., Deeming, T.: Astrophysics I. Jones and Bartlett Publishers. Sudbury, 1984.
  • 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
  • EMERSON, D. Interpreting astronomical spectra. Chichester: John Wiley & Sons, 1996, vii, 461 s. ISBN 0-471-94176-X. info
Language of instruction
Czech
Further Comments
The course is taught annually.
The course is taught every week.
  • Enrolment Statistics (recent)
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