Astronomy and Astrophysics – Astronomy
Scientific paper
May 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...427l..51o&link_type=abstract
Astrophysical Journal, Part 2 - Letters, vol. 427, no. 1, p. L51-L54
Astronomy and Astrophysics
Astronomy
11
Abundance, Carbon Compounds, Interstellar Matter, Methylene, Molecular Clouds, Radio Astronomy, Radio Spectra, Rotational Spectra, Astronomical Observatories, High Resolution, Radio Telescopes
Scientific paper
We have detected a new interstellar molecule, H2CN (methylene amidogen), in the cold, dark molecular cloud TMC-1. The column density of H2CN is estimated to be approximately 1.5 x 1011 cm-2 by assuming an excitation temperature of 5 K. This column density corresponds to a fractional abundance relative to H2 of approximately 1.5 x 10-11. This value is more than three orders of magnitude less than the abundance of the related molecule HCN in TMC-1. We also report a tentative detection of H2CN in Sgr B2(N). The formation mechanism of H2CN is discussed. Our detection of the N2CN molecule may suggest the existence of a new series of carbon-chain molecules, CH2C(n)N (N = 0, 1, 2, ...).
Irvine William M.
McGonagle Douglas
Ohishi Masatoshi
Saito Shuji
Yamamoto Satoshi
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