Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
University of Texas
California, University, Berkeley, Calif.
Texas Univ., Austin.
California Institute of Technology, Pasadena, CA
California Institute of Technology, Pasadena.
Department of Astronomy, University of Texas, Austin, TX, USA;
Astronomy, University of Texas, Austin, TX, USA;
California, University, Berkeley, CA
UT- Austin
University of Texas at Austin
University of California at Davis
Caltech
Department of Astronomy, University of Texas at Austin, RLM 15.308, C-1400 Austin, TX 78712-1083, USA
Palomar Observatory, Pasadena, CA
UT-Austin
The University of Texas at Austin
UT Austin
Department of Astronomy, University of Texas, Austin, TX 78712
Texas, University, Austin
Department of Astronomy and McDonald Observatory, University of Texas
California Inst. of Technol., Pasadena
Department of Astronomy, University of Texas at Austin, TX 78712-1083, USA
Texas, University, Austin, TX; California, University, Berkeley; Palomar Observatory, Pasadena, CA
California, University, Berkeley, CA; Hawaii, University, Hilo, HI
Texas, University, Austin, TX; California, University Berkeley, CA
Department of Astronomy, University of Texas, RLM 15.308, Austin, TX 78712, USA
University of Texas, Austin, TX, US
Department of Astronomy, University of Texas at Austin, RLM 15.308, C-1400, Austin, TX 78712-1083, USA
Dept. of Ast., U. of Texas
University of Texas at Austin, Department of Astronomy, Austin, TX 78712, USA; Visiting Astronomer at the Infrared Telescope Facility, which is operated by the University of Hawaii under cooperative agreement NCC 5-538 with the National Aeronautics and Space Administration, Office of Space Science, Planetary Astronomy Program.
Department of Astronomy, University of Texas, Austin, Texas
University of Texas at Austi
10 Micrometer Infrared Camera
4.6 micron absorption features due to solid phase CO and cyano group molecules toward compact infrared sources
4.6 micron absorption features due to solid phase CO toward compact infrared sources
A Decade Of Teacher Professional Development With SOFIA's EXES And TEXES
A Detailed Analysis of the Dust Formation Zone of IRC+10216 Derived from Mid-IR Bands of C2H2 and HCN
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