The Oxygen Isotopic Composition of the Solar System in a Galactic Context: New Results for Co in Young Stellar Objects and Implications for the Birth Environment of the Solar System
نویسندگان
چکیده
NEW RESULTS FOR CO IN YOUNG STELLAR OBJECTS AND IMPLICATIONS FOR THE BIRTH ENVIRONMENT OF THE SOLAR SYSTEM. E. D. Young , M. Gounelle, R. L. Smith , M. R. Morris, and K. M. Pontoppidan, Department of Earth and Space Sciences, University of California Los Angeles (UCLA), Los Angeles, CA 90095, USA, Institute of Geophysics and Planetary Physics, UCLA ([email protected]), Laboratoire d’Étude de la Matière Extraterrestre, Muséum National d’Histoire Naturelle, 57 rue Cuvier, CP52, 75005 Paris, France, Department of Physics and Astronomy, UCLA, Hubble Fellow, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA
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