Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
NASA / Ames
NASA Ames Research Center
University of Illinois Observatory, USA
SETI Enterprises, Moffett Field, CA, US
NASA. Ames Research Center, Moffett Field, CA, US
NASA Ames Research Center, Moffett Field, California, US
NASA Ames Research Center, MS 245-6, Moffett Field, CA 94035 Univ., Los Angeles
NASA / Ames Research Center, Moffett Field, CA 94035-1000, USA; Orion Enterprises, M.S. 245-6, Moffett Field, CA 94035-1000, USA
NASA / Ames, Orion Enterprises
National Radio Astronomy Observatory, Green Bank, WV, USA
NASA Ames Research Center, M.S. 245-6, Moffett Field, CA 94035-1000, USA
NASA, Ames Research Center; SETI Inst., Moffett Field, CA
NASA, Ames Research Center, Moffett Field; Orion Enterprises, Mountain View, CA
NASA Ames Research Center, Mail Stop 245-6, Moffett Field, CA 94035-1000, USA; Orion Enterprises
NASA / Ames Research Center, Moffett Field, CA 94035-1000, USA; Orion Enterprises, MS 245-6, Moffett Field, CA 94035-1000, USA
NASA, Ames Research Center, Moffett Field, CA
Chicago Univ., Chicago, IL, US
NASA, Ames Research Center, Moffett Field; California, University, Los Angeles
NASA-ARC
National Aeronautics and Space Administration. Ames Research Center, Moffett Field, CA.
NASA, Ames Research Center, Astrophysical Experiments Branch, Moffett Field; California, University, Los Angeles, CA
NASA Ames Research Center, M.S. 245-6, Moffett Field, CA 94035-1000, USA ; Orion Enterprises
NASA Ames Research Center, Moffett Field, CA 94035-1000, USA; Orion Enterprises, M.S. 245-6, Moffett Field, CA 94035-1000, USA; Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China
California State University, Fullerton, Calif.
NASA / Ames Research Center, MS 245-6,
$^{12}$C/$^{13}$C ratio in planetary nebulae from the IUE archives
A bipolar outflow of ionized gas in K3-50A: H76 alpha radio recombination line and continuum observations of K3-50
A Blister Model for the Orion Nebula
A Discussion of the Sizes and Excitation of H II Regions
A Far-Infrared Spectral Line Survey of 23 Disk Galaxies
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