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Others:  () 
Credits  Dept. 

5.625 (4.5 ECTS)  UV 
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Others:  () 
In this course, students should gain a basic insight on those (magneto) hydrodynamic processes governing the formation and evolution of astrophysical objects and cosmological inhomogeneities, paying particular attention to understand the corresponding equations and algorithms to solve them. The course will be rather theoretical and will be the basis for the subject "Applications of Computational Astrophysics".
Estimated time (hours):
T  P  L  Alt  Ext. L  Stu  A. time 
Theory  Problems  Laboratory  Other activities  External Laboratory  Study  Additional time 

T  P  L  Alt  Ext. L  Stu  A. time  Total  

1,0  0  0  0  0  0  0  1,0 

T  P  L  Alt  Ext. L  Stu  A. time  Total  

12,0  0  0  0  0  6,0  0  18,0 

T  P  L  Alt  Ext. L  Stu  A. time  Total  

10,0  0  8,0  6,0  0  4,0  2,0  30,0  


T  P  L  Alt  Ext. L  Stu  A. time  Total  

1,0  0  0  10,0  0  10,0  0  21,0  

Total per kind  T  P  L  Alt  Ext. L  Stu  A. time  Total 
30,0  0  14,0  20,0  0  28,0  4,0  96,0  
Avaluation additional hours  0  
Total work hours for student  96,0 
Classes will build up concepts in a structured fashion. The basic theoretical background in the lectures will consolidated by means of practical exercises. The practical work will consist on computer practices where the student will use programs provided by the lecturer, public domain programs appropriately documented or programs that will be developed by the student. The contents of the course will be available online.
The evaluation of the course will be based on the work developed by the students in the practical part (problems).
Calculus (differential and integral). Fortran (basic level).