Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
NASA / Ames Research Center
National Aeronautics and Space Administration. Ames Research Center, Moffett Field, CA.
Planetary Science Inst., Tucson, Ariz.
Johns Hopkins Univ., Baltimore, MD, US
NASA, Ames Research Center, Moffett Field, CA
Space Science Division, Mail Stop 245-6, NASA Ames Research Center, Moffett Field, CA 94035-1000 Branch, NASA Ames Research Center, MS 245-6, Moffett Field, CA 94035; Adjunct Astronomer, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218
NASA Ames Research Ctr., USA
Space Science and Astrophysics Branch, NASA Ames Research Center, MS 245-6, Moffett Field, CA 94035, USA
NASA Ames Research Center
ASTRON Dwingeloo
NASA, Ames Research Center, Space Science Div., Moffett Field; California, University, Santa Cruz, Calif.
Lick Observatory, Santa Cruz, Calif.
NASA, Ames Research Center, Space Sciences Div., Moffett Field, Calif.
NASA / ARC
NASA, Ames Research Center, Moffett Field, Calif.
Stichting Radiostraling van Zon en Melkweg, Dwingeloo, Netherlands
Dwingeloo, Radiosterrenwacht, Dwingeloo, Netherlands
NASA. Ames Research Center, Moffet Field, CA, US
NASA. Ames Research Center, Moffett Field, CA, US
California Univ., Berkeley.
Leiden Univ., Netherlands
NASA Ames Research Center, Moffett Field, CA 94035, USA Sterrewacht, Westerbork, Netherlands
NASA, Ames Research Center, Space Science Div., Moffett Field, CA
NASA, Ames Research Center, Space Sciences Div., Moffett Field; Lick Observatory, Santa Cruz, Calif.
Radio Sterrenwacht, Westerbork, Netherlands
Dwingeloo, Radiosterrenwacht, Netherlands
NASA, Ames Research Center, Astrophysical Experiments Branch, Moffett Field, CA
0.68 to 5.2 Micron Observations and Analysis of Non-Mira S Stars
1-13 Micron Spectroscopy of SN1987A
3 micron spectrophotometry of Comet Halley - Evidence for water ice
3-12-um images of HD44179 and M42: spectral differencing as a mid-infrared astronomical image enhancement technique
3.3 and 11.3 micron images of HD 44179 - Evidence for an optically thick polycyclic aromatic hydrocarbon disk
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