Astrophys. J., 812, L5 (2015/October-2)
Interstellar detection of methyl isocyanate CH3NCO in Sgr B2(N): a link from molecular clouds to comets.
HALFEN D.T., ILYUSHIN V.V. and ZIURYS L.M.
Abstract (from CDS):
A new interstellar molecule, CH3 NCO (methyl isocyanate), has been detected using the 12 m telescope of the Arizona Radio Observatory (ARO). CH3NCO was identified in spectra covering 48 GHz (68-116 GHz) in the 3 mm segment of a broadband survey of Sgr B2(N). Thirty very favorable rotational lines (Ka= 0 and Ka= 1 only; Eu< 60 K) originating in five consecutive transitions (J = 8 7, 9 8, 10 9, 11 10, and 12 11) in both the A and E internal rotation species are present in this frequency range. Emission was observed at all of the predicted frequencies, with 17 lines appearing as distinct, uncontaminated spectral features, clearly showing the classic a-type, asymmetric top pattern, with ≈ 20-70 mK. The CH3NCO spectra also appear to exhibit two velocity components near VLSR≈ 62 and 73 km/s, both with ΔV1/2≈ 10 km/s–typical of molecules such as CH2CHCN, HNCO, and HCOOCH3in Sgr B2(N). The column density of CH3NCO in Sgr B2(N) was determined to be Ntot≈ 2.3x1013 and 1.5x1013/cm2 for the 62 and 73 km/s components, corresponding to fractional abundances, relative to H2, of f ≈ 7.6x10–12 and 5.0x10–12, respectively. CH3 NCO was recently detected in volatized material from comet 67P/Churyumov-Gerasimenko by Rosetta's Philae lander, with an abundance ∼1.3% of water; in Sgr B2(N), CH3NCO is roughly ∼0.04% of the H2O abundance.
astrochemistry - comets: individual: 67P,Churyumov-Gerasimenko - ISM: molecules - line: identification - methods: laboratory: molecular - molecular data
VizieR on-line data:
<Available at CDS (J/ApJ/812/L5): table1.dat table3.dat>
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