Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
Scientist
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA; School of Engineering & Applied Sciences, Harvard University, 29 Oxford St., Cambridge, MA 02138, USA; Also at: Institute for Theoretical Chemistry, Departments of Chemistry and Biochemistry, The University of Texas at Austin, Austin, TX 78712, USA
Institute for Theoretical Chemistry, Department of Chemistry and Biochemistry, University of Texas at Austin, Austin, Texas 78712
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA, and Division of Engineering and Applied Sciences, Harvard University, 29 Oxford Street, Cambridge, MA 02138, USA; Institute for Theoretical Chemistry, Department of Chemistry and Biochemistry, The University of Texas, Austin, TX 78712, USA
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; and School of Engineering and Applied Sciences, Harvard University, 29 Oxford Street, Cambridge, MA 02138; Also at Institute for Theoretical Chemistry, Departments of Chemistry and Biochemistry, University of Texas at Austin, Austin, TX 78712. Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; and Division of Engineering and Applied Sciences, Harvard University, 29 Oxford Street, Cambridge, MA 02138; Also at Institute for Theoretical Chemistry, Department of Chemistry and Biochemistry, University of Texas at Austin, Austin, TX 78712. Center for Astrophysics, Cambridge, MA; and Division of Engineering and Applied Sciences, Harvard University, Cambridge, MA; Also at Institute for Theoretical Chemistry, Department of Chemistry and Biochemistry, The University of Texas, Austin, TX. cg
A submillimeter study of CH in Orion KL
A Survey of C4H, C6H, and C6H- With the Green Bank Telescope
CH+(1-0) and 13CH+(1-0) absorption lines in the direction of massive star-forming regions
Contrasting [CII], methylidynium ion CH^+, and methanol physical and chemical tracers around Orion KL.
Detection of hydrogen fluoride absorption in diffuse molecular clouds with Herschel/HIFI: a ubiquitous tracer of molecular gas
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