Changes between Version 100 and Version 101 of SavinGroup/MergedBeams


Ignore:
Timestamp:
10/07/09 16:52:32 (17 years ago)
Author:
kmiller@…
Comment:

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  • SavinGroup/MergedBeams

    v100 v101  
    22= Ion-Atom collisions =
    33[[br]]
    4 We are measuring rate coefficients of the reaction H^^-^^ + H = H,,2,, . [[br]]This is an important mechanism for forming H,,2,, molecules which act as a coolant in primordial clouds.[[br]] This cooling effect is necessary in the formation of the first stars.[[Image(https://docs.astro.columbia.edu/attachment/wiki/SavinGroup/MergedBeams/First Star.png?format=raw, 50%, right)]]`                                                                    Abel et al, Science 2002`
     4We are measuring rate coefficients of the reaction H^^-^^ + H = H,,2,,. This is an important mechanism for forming H,,2,, molecules which act as a coolant in primordial clouds.[[br]] This cooling effect is necessary in the formation of the first stars.[[Image(https://docs.astro.columbia.edu/attachment/wiki/SavinGroup/MergedBeams/First Star.png?format=raw, 50%, right)]]`                                                                    Abel et al, Science 2002`
    55[[br]]
    66[[br]]