Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Caltech
California Institute of Technology, Geological and Planetary Sciences, 1200 E. California Blvd, Pasadena, CA 91125, USA
Research Center for Environmental Changes, Academia Sinica, Taipei 115, Taiwan; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA
Graduate Institute of Astronomy, National Central University, Jhongli, Taiwan
Research Center for Environmental Changes, Academia Sinica, Taipei 115, Taiwan; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125.
Research Center for Environment Changes, Academia Sinica, Taipei, Taiwan; Graduate Institute of Astronomy, National Central University, Jhongli, Taiwan
Academia Sinica and Caltech
Division of Geological and Planetary Sciences, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125.
Academia Sinica, Taiwan
Research Center for Environmental Changes, Academia Sinica, Taipei 11529, Taiwan
Research Center for Environmental Change, Academia Sinica, Taipei, Taiwan ; Graduate Institute of Astronomy, National Central University, Jhongli, Taiwan ; Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan
Research Center for Environmental Changes and Institute of Astronomy and Astrophysics, Academia Sinica, Taipei 115, Taiwan; Graduate Institute of Astronomy, National Central University, Jhongli, Taiwan
Research Center for Environmental Changes, Academia Sinica, Taipei, Taiwan
Graduate Institute of Astronomy, National Central University, Jhongli City, Taiwan
Division of Geological and Planetary Science, California Institute of Technology; Research Center for Environmental Changes, Academia Sinica
Research Center for Environmental Changes, Academia Sinica, Taipei, Taiwan; Graduate Institute of Astronomy, National Central University, Jhongli, Taiw
A Born-Oppenheimer photolysis model of N2O fractionation
A Crossed Molecular Beams Study on the Formation of the Exotic Cyanoethynyl Radical in Titan's Atmosphere
A size of ~1 AU for the radio source Sgr A* at the centre of the Milky Way
Absorption Cross Sections of NH3, NH2D, NHD2, and ND3 in the Spectral Range 140-220 nm and Implications for Planetary Isotopic Fractionation
Aerosol distribution and physical properties in the Titan atmosphere
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