Určování rozložení hmoty v jádře Galaxie z pohybů hvězd
We present an implementation of the statistical approach to the stars-gas mass exchange cycle into an N-body code. First, we summarize available data on stellar mass-loss and derive the time-dependency of the mass-loss rate of a single stellar population. Since the adopted probabilistic scheme that...
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| Format: | Dissertation |
| Language: | Czech |
| Published: |
2007
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| Online Access: | http://www.nusl.cz/ntk/nusl-288440 |