A search for HCOCN in molecular clouds

Details A search for HCOCN in molecular clouds A search for HCOCN in molecular clouds

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...224l..24g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 224, no. 1-2, Oct. 1989, p. L24-L26.

Astronomy and Astrophysics

Astrophysics

2

Astronomical Spectroscopy, Cyano Compounds, Interstellar Chemistry, Molecular Clouds, Molecular Ions, Brightness Temperature, Formaldehyde, Interstellar Matter

Scientific paper

Among the numerous chemical species found in the ISM, there are a few examples of pairs of molecules formed by the substitution of an H atom by a CN radical. Since formaldehyde H2CO is a fairly abundant and ubiquitous molecule, a search for the CN-substituted HCOCN toward the molecular sources SgrB2(OH) and Orion-IRc2 was conducted. No convincing evidence for this new interstellar species is found down to an abundance of 5 x 10 to the -11th and 7 x 10 to the -11th in these two sources, respectively.

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