An upper limit to the acetylene abundance toward BN in the orion molecular cloud

Details An upper limit to the acetylene abundance toward BN in the orion molecular cloud An upper limit to the acetylene abundance toward BN in the orion molecular cloud

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...345..265k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 345, Oct. 1, 1989, p. 265-267.

Astronomy and Astrophysics

Astrophysics

1

Abundance, Acetylene, Interstellar Chemistry, Molecular Clouds, Orion Nebula, Absorption Spectra, Carbon Monoxide, Infrared Spectra, Interstellar Gas

Scientific paper

A search for the acetylene (C2H2) nu3 infrared vibration-rotation
absorption near 3 microns toward the Becklin-Neugebauer source in the
Orion molecular cloud is reported. The relative abundance of C2H2/CO in
the quiescent gas is less than 0.003.

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