Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
SMTO University of Arizona
Joint Astronomy Centre
SMTO-Steward Observatory
James Madison University
SMTO - Steward Observatory
JAC
University of Arizona, SMTO
National Research Council, British Columbia, Canada
SMTO, Tucson
Department of Physics and Astronomy, James Madison University, Harrisonburg, VA 22807, USA / NASA-ARC
Submillimeter Telescope Observatory, Steward Observatory, University of Arizona, Tucson, AZ 85721
University of Arizona / STO
CIW, DTM
DTM-CIW
Joint Astronomy Centre, University Park, Hilo, HI 96720 Observatory, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ, USA
Department of Terrestrial Magnetism, Carnegie Institution of Washington
Joint Astronomy Centre, University Park, Hilo, HI 96720; Department of Physics, James Madison University, Harrisonburg, VA 22807-7702. Astronomy Center, 660 North A'ohōkū Place, University Park, Hilo, HI 96720.
SMTO-Steward Observatory, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USA
NASA Ames
NASA / Ames Research Center
James Madison Univ
Steward Observatory SMTO, University of Arizona, Tucson, Arizona
NASA. Ames Research Center, Moffit Field, CA, US
Steward Observatory, University of Arizona, Tucson, AZ 85721
Submillimeter Telescope Observatory, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USA
NASA, Ames Research Center, Moffett Field, CA
NASA Ames Research Center
Carnegie Institute of Technology
Texas, University, Austin
DTM - Carnegie Institution of Washington
Steward Observatory, University of Arizona
NASA, Ames Research Center, Moffett Field, CA; Texas, University, Austin
Submillimeter Telescope O
"Complete" models of young stellar objects: the spectral energy distributions of embedded YSO's with and without disks.
'Spherical' disks: Moving toward a unified source model for L1551
10 MU m\ Spectroscopy of Comet C/1996 Q1 (Tabur)
A dust ring around Epsilon Eridani: analogue to the young Solar System
A Multiwavelength Study of Outflows in OMC-2/3
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Profile ID: LFWR-SCP-P-49590