On Origin of Xe-HL in Meteoritic Nanodiamonds

Details On Origin of Xe-HL in Meteoritic Nanodiamonds On Origin of Xe-HL in Meteoritic Nanodiamonds

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1007u&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Computer Science

1

Scientific paper

The Xe-HL component is shown to be formed and captured simultaneously
with the nanodiamond synthesis in the conditions of shock wave
propagation from supernova explosions, and its isotopic composition is
an effect of acceleration in the shock waves.

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