Exploring Phy575 Chapter 6 Part 2
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- ... see this equation this is the equation of mass conservation or continue so basically it tells you that given a
- Stellar Structure revision (part 1)
- Deriving the equation of hydrostatic equilbrium of a star.
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- Considering that epsilon is proportional to r to the power
In-Depth Information on Phy575 Chapter 6 Part 2
This topic will cover the process of death of stars in the case of low massive and high massive stars. In which we learn how much matter is inside stars, and how we find that out (we can't put them on a beam balance, isn't it?) Fluid Mechanics; Derivaiton of Mass Conservation Equations; Derivation of Continuity Equation. The cycle of a star - Episode - 2( Hydrostatic equilibrium, main sequence star, HR diagram)
If none then let me proceed to the next
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