Documents Star formation from (local) molecular clouds to spiral arms Lee Hartmann University of Michigan.

Slide 1 Star formation from (local) molecular clouds to spiral arms Lee Hartmann University of Michigan Slide 2 Structure of molecular clouds Efficiency of star formation…

Documents Stellar Formation

Inter Stellar Matter with a high enough density, and a low enough temperature for proto-stars to form. Protostars form in cold dark nebulae Star Formation Giant Molecular…

Documents Inter Stellar Matter with a high enough density, and a low enough temperature for proto-stars to...

Inter Stellar Matter with a high enough density, and a low enough temperature for proto-stars to form. Protostars form in cold dark nebulae Star Formation Giant Molecular…