Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138 and Division of Engineering and Applied Sciences, Harvard University, Cambridge, Massachusetts 02138
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
I. Physikalisches Institut, Universität zu Köln,50937 Köln, Germany
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
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 Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA; School of Engineering and Applied Sciences, Harvard University, 29 Oxford St., Cambridge, MA 02138, USA; Laboratoire de Chimie Physique Moléculaire, École Polytechnique Fédérale de Lausanne, Station 6, CH-1015 Lausanne, Switzerland.
I. Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, 50937 Köln, Germany
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA; School of Engineering & Applied Sciences, Harvard University, 29 Oxford Street, Cambridge, MA 02138, USA; Laboratoire de Chimie Physique Moléculaire, École Polytechnique Fédérale de Lausanne, Station 6, CH-1015 Lausanne, Switzerland.
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; and Division of Engineering and Applied Sciences, Harvard University, Cambridge, MA Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; and School of Engineering and Applied Sciences, Harvar
A Concise New Look at the l-Type Spectrum of H12C14N
Accurate rotational spectroscopy of sulfur dioxide, SO2, in its ground vibrational and first excited bending states, v2 = 0, 1, up to 2 THz
An Interferometric 270--355 GHz Spectral Line Survey of the Red Supergiant VY CMa
Analysis of New Data Sets Pertaining to the Water Molecule
Analysis of the Rotational Spectrum of HDO in its v_2 = 0 and 1 Vibrational States up to 2.8 THz
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