Stellar Evolution Clusters Matching a young, metal rich star an old, metal poor

Question

Stellar Evolution Clusters Matching a young, metal rich star an old, metal poor star the position on the HR diagram of stars that have just begun to fuse hydrogen in their cores the path followed on the HR diagram by a point representing an evolving star the tear-drop shaped regions around each star in a binary star system inside of which gas is gravitationally bound to that star the upper limit to the mass of a white dwarf; 1.4 solar masses helium fusion that occurs in a thin shell surrounding the core of a star the balance of fusion pressure and gravity in a star on the main sequence the mechanism for keeping track of how the energy is used in the formation stages of stellar evolution evolutionary track population I population II Roche lobe zero-age main sequence (ZAMS) Chandrasekhar limit hydrostatic equilibrium helium shell fusion virial theorem

Explanation / Answer

1. Poplulation 1

2. Population 2

3. ZAMS

4. Evolutionary track

5. Roche lobe

6. Chadrasekhar limit

7.Helium shell fusion

8.Hydrostatic equilibrium

9.viral theorem

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