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Updated: Jul 22, 2026

Improved Heterojunction Quality in Cu2O-based Solar Cells Through the Optimization of Atmospheric Pressure Spatial Atomic Layer Deposited Zn1-xMgxO
08:14

Improved Heterojunction Quality in Cu2O-based Solar Cells Through the Optimization of Atmospheric Pressure Spatial Atomic Layer Deposited
Zn1-xMgxO

Published on: July 31, 2016

El origen de la nube molecular para la heterogeneidad de isótopos de oxígeno en el sistema solar

Hisayoshi Yurimoto1, Kiyoshi Kuramoto

  • 1Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Meguro, Tokyo 152-8551, Japan. yuri@geo.titech.ac.jp

Science (New York, N.Y.)
|September 18, 2004
PubMed
Resumen

Los isótopos anómalos de oxígeno en los meteoritos probablemente se originaron a partir de la fotodissociación ultravioleta en la nube molecular madre. Los granos de polvo helado transportaron estos materiales a la nebulosa solar, enriqueciendo el gas del disco interno.

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