Changes between Version 86 and Version 87 of SavinGroup/MergedBeams


Ignore:
Timestamp:
10/07/09 15:56:43 (17 years ago)
Author:
kmiller@…
Comment:

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  • SavinGroup/MergedBeams

    v86 v87  
    22= Ion-Atom collisions =
    33[[br]]
    4 We 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. This cooling effect is necessary in the formation of the first stars.
     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. This cooling effect is necessary in the formation of the first stars.
    55[[br]]
    6 `         `[[br]][[Image(https://docs.astro.columbia.edu/attachment/wiki/SavinGroup/MergedBeams/First Star.png?format=raw, 50%)]]
     6`         `[[Image(https://docs.astro.columbia.edu/attachment/wiki/SavinGroup/MergedBeams/First Star.png?format=raw, 50%)]]
    77[[br]]
    88[[br]]