765649S

Astrophysics

 

an advanced course (10 credits)

at the Space Physics and Astronomy research unit, University of Oulu

The course period: January 7 – April 24, 2026

Lectures, exercise and practical sessions take place usually on Monday, Wednesday, and Thursday at 14-16, see Peppi for detail. However, classes on Thursday will only occur when I announce them!

The course is lectured in English

Teacher: Vitaly Neustroev, MA 308, vitaly[-at-]neustroev.net

Assistent: Paula Kvist, paula.kvist [-at-] oulu.fi

 


 

Course plan:

  • Stellar structure and evolution
  • Radiative processes
  • Stellar photospheres
  • Interstellar Medium
  • etc…

Theoretical and practical considerations will be supplemented with the home exercises which constitute the important part of the course.

 

Literature:

Textbook choice for this course is largely a matter of personal taste. I provide below a list of recommended books. Study them in parallel with the lectures.

 

Compulsory problems (return by the deadline). 5+ sets (30% of the final score).


 

Schedule

  • Lecture 1: January 7: Introduction (What is Astrophysics and Theoretical Astrophysics? Astronomical units). Stars (Role of stars; Definition; What can we learn from observations?).
    PDF
  • January 8: NO CLASS
  • Lecture 2: January 14: Stars (Properties of stars; Stellar timeline; basic assumptions, mass conservation, hydrostatic equilibrium).
    PDF
  • Lecture 3: January 19: Stars (Virial theorem. Timescales of stellar evolution. Conditions in stellar interiors).
    PDF
  • Lecture 4: January 21: Stars (Energy generation. The equation of conservation of energy). Basics about radiative transfer (Specific intensity. Absorption coefficient).
    PDF
  • Lecture 5: January 22: Basics about radiative transfer (Radiation terms, specific intensity, interaction radiation – matter, parallel-ray radiative transfer equation, solution of the parallel-ray RTE)
    PDF
    Compulsory problems: Set 1 (return by January 28).
  • Lecture 6: January 26: Basics about radiative transfer (Mean Intensity, Flux, and K-integral. RTE in plane-parallel atmosphere. The temperature gradient for radiative transport). The equations of stellar structure and possible ways to solve them. Boundary conditions.
    PDF
  • Lecture 7: January 28: Convection and conditions for its occurrence. Equation of state (EOS). Degeneracy pressure.
    PDF
  • Exercise session: January 29:

    starts at 14:30