Excitation of interstellar molecules in the Ori-KL source

Details Excitation of interstellar molecules in the Ori-KL source Excitation of interstellar molecules in the Ori-KL source

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..405o&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astronomy

10

Interstellar Gas, Molecular Clouds, Molecular Excitation, Orion Nebula, Radial Velocity, Radio Sources (Astronomy), Interstellar Masers, Molecular Spectra, Spectral Line Width

Scientific paper

A molecular spectral line survey of the title source detected 166 molecular lines from 18 interstellar molecules in the frequency ranges of 34.25 - 50.00, 83.50 - 84.50, and 86.00 - 91.50 GHz. For each molecule, gaussian decomposition of the velocity components in the transition profiles gave consistent radial velocity and linewidth. Rotation diagrams were drawn for each velocity component.

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