Adsorption of Water Gas on to Grains in the Accretion Disk as a Source of Inner Solar System Water: Direct Evidence from Monte Carlo Simulation

Details Adsorption of Water Gas on to Grains in the Accretion Disk as a Source of Inner Solar System Water: Direct Evidence from Monte Carlo Simulation Adsorption of Water Gas on to Grains in the Accretion Disk as a Source of Inner Solar System Water: Direct Evidence from Monte Carlo Simulation

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007m%26psa..42.5230m&link_type=article

70th Annual Meteoritical Society Meeting, held in August 13-17, 2007, Tucson, Arizona. Meteoritics and Planetary Science Supplem

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