Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
Scientist
Extrasolar Research Corporation
National Center for Atmospheric Research, Boulder, Colo.
Washington Univ., Seattle.
Cal. State University at Los Angeles
Jet Propulsion Lab., California Institute of Technology, Pasadena, CA.
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, US
Extrasolar Research Corporation, 720 Magnolia Avenue, Pasadena, CA 91106
High Altitude Observatory, Boulder, CO
Department of Physics and Astronomy, 5151 State University Drive, California State University, Los Angeles, CA 90032
California Inst. of Technology; JPL, Pasadena
California State University, Los Angeles
IPAC, Caltech
Owens Valley Radio Observatory, Pasadena, CA
California State University at Los Angeles
Jet Propulsion Lab., Cal Tech., Pasadena, CA, US
Extrasolar Research Corp.
IPAC
Extrasolar Research Corporation, 569 South Marengo Avenue, Pasadena, CA 91101
Cal State Los Angeles
California Univ., Berkeley
High Altitude Observatory; National Center for Atmospheric Research, Boulder, CO
JPL, Pasadena, CA
IGN, Guadalajara, Spain
Extrasolar Research Co.
Cal State LA
CSULA
JPL, Pasadena, CA; Canadian Institute for Theoretical Astrophysics, Toronto, Canada
JPL; California Inst. of Technology, Pasadena
Toronto, University, Canada
California State University- Los Angeles
Cal. State Univ. at Los Angeles
Infrared Processing and Analysis Center, Jet Propulsion Laboratory and California Institute of Technology
California, University, Berkeley, CA
Cal State University Los Angeles
Department of Physics and Astronomy, California State University, 5151 State University Drive, Los Angeles, CA 90032-8206; Extrasolar Research Corporation, 2026 Hall Canyon Drive, La Cañada, CA 91011.
IPAC; JPL and Caltech
California Institute of Technology, Pasadena
CalStateLA
10 Micron Search for Cool Companions of Nearby Stars
10 Micron Search for Cool Companions of Nearby Stars
A Candidate Protoplanet in the Taurus Molecular Cloud
A Candidate Protoplanet in the Taurus Star Forming Region
A correlation between the IRAS infrared cirrus at 60 or 100 microns and neutral atomic hydrogen in the outer galaxy
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Profile ID: LFWR-SCP-P-110676