Changes between Version 96 and Version 97 of SavinGroup/MergedBeams


Ignore:
Timestamp:
10/07/09 16:51:23 (17 years ago)
Author:
kmiller@…
Comment:

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  • SavinGroup/MergedBeams

    v96 v97  
    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.
    5 [[br]][[br]][[br]]
    6 [[br]]
     4We 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. This cooling effect is necessary in the formation of the first stars.
     5
    76`                         `[[Image(https://docs.astro.columbia.edu/attachment/wiki/SavinGroup/MergedBeams/First Star.png?format=raw, 50%, right)]]`                                                                    Abel et al, Science 2002`
    87[[br]]