Stellar evolution for students of the Moscow University

Details Stellar evolution for students of the Moscow University Stellar evolution for students of the Moscow University

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iauss...2e..34k&link_type=abstract

Innovation in Teaching/Learning Astronomy Methods, 26th meeting of the IAU, Special Session 2, 17-18 August, 2006 in Prague, Cze

Computer Science

Learning

Scientific paper

The theory of stellar interior is a very stimulating tool of the physical and astrophysical curricula. To support the corresponding lecture courses, a practical work was proposed and elaborated upon in 1991 for advanced students of the physics department who specialized in astrophysics at Moscow State University. The work is recommended for 5th year students and requires significant knowledge of theoretical astrophysics. The main purpose of the work is to calculate the evolutionary set of stellar models, including those for the Sun. The PC program is based on the B. Paczynski set of routines and supported by the WEB interface. This allows working via Internet. The results of the work may be presented both in a table and graph forms.

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