Low-Pressure Formation Routes for Interstellar Microdiamonds: Chemical Vapor Deposition vs. Homogeneous Nucleation

Details Low-Pressure Formation Routes for Interstellar Microdiamonds: Chemical Vapor Deposition vs. Homogeneous Nucleation Low-Pressure Formation Routes for Interstellar Microdiamonds: Chemical Vapor Deposition vs. Homogeneous Nucleation

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996m%26psa..31q..24b&link_type=gif

Meteoritics & Planetary Science, vol. 31, page A24

Physics

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