Observational properties of stars, gas hydrodynamics, mass-luminosity relation, nucleosynthesis and stellar evolution.
SH2401 Stellar Structure and Evolution 6.0 credits
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Course syllabus as PDF
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Course syllabus SH2401 (Autumn 2007–)Content and learning outcomes
Course contents
Intended learning outcomes
The student should have obtained an understanding of the observational properties of stars and be able to explain the physical principles underlying the structure and evolution of stars. Nucleosynthesis and its dependence on mass are also studied.
Literature and preparations
Specific prerequisites
Recommended prerequisites: Previous knowledge of mathematics, physics and measuring techniques.
Literature
Christensen-Dalsgard: Stellar Structure and Evolution (booklet)
Examination and completion
Grading scale
Examination
- TEN1 - Examination, 6.0 credits, grading scale: A, B, C, D, E, FX, F
Based on recommendation from KTH’s coordinator for disabilities, the examiner will decide how to adapt an examination for students with documented disability.
The examiner may apply another examination format when re-examining individual students.
If the course is discontinued, students may request to be examined during the following two academic years.
Other requirements for final grade
One written exam (TENA; 6 university credits)
Examiner
Ethical approach
- All members of a group are responsible for the group's work.
- In any assessment, every student shall honestly disclose any help received and sources used.
- In an oral assessment, every student shall be able to present and answer questions about the entire assignment and solution.