We report the detection of the pre-biotic molecule CH3NCO in a solar-type protostar, IRAS16293-2422 B. A significant abundance of this species on the surface of the comet 67P/Churyumov-Gerasimenko has been proposed, and it has recently been detected in hot cores around high-mass protostars. We observed IRAS16293-2422 B with the Atacama Large Millimeter Array in the 90 to 265 GHz range, and detected eight unblended transitions of CH3NCO. From our Local Thermodynamic Equilibrium analysis, we derived an excitation temperature of 110 +/- 19 K and a column density of (4.0 +/- 0.3) x 10(15) cm(-2), which results in an abundance of <=(1.4 +/- 0.1) x 10(-10) with respect to molecular hydrogen. This implies a CH3NCO/HNCO and CH3NCO/NH2CHO column density ratios of similar to 0.08. Our modelling of the chemistry of CH3NCO suggests that both ice surface and gas phase formation reactions of this molecule are needed to explain the observations.
Martin-Domenech, R., Rivilla, V.M., Jimenez-Serra, I., Quenard, D., Testi, L., Martin-Pintado, J. (2017). Detection of methyl isocyanate (CH3NCO) in a solar-type protostar. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 469(2), 2230-2234 [10.1093/mnras/stx915].
Detection of methyl isocyanate (CH3NCO) in a solar-type protostar
Testi, L;
2017
Abstract
We report the detection of the pre-biotic molecule CH3NCO in a solar-type protostar, IRAS16293-2422 B. A significant abundance of this species on the surface of the comet 67P/Churyumov-Gerasimenko has been proposed, and it has recently been detected in hot cores around high-mass protostars. We observed IRAS16293-2422 B with the Atacama Large Millimeter Array in the 90 to 265 GHz range, and detected eight unblended transitions of CH3NCO. From our Local Thermodynamic Equilibrium analysis, we derived an excitation temperature of 110 +/- 19 K and a column density of (4.0 +/- 0.3) x 10(15) cm(-2), which results in an abundance of <=(1.4 +/- 0.1) x 10(-10) with respect to molecular hydrogen. This implies a CH3NCO/HNCO and CH3NCO/NH2CHO column density ratios of similar to 0.08. Our modelling of the chemistry of CH3NCO suggests that both ice surface and gas phase formation reactions of this molecule are needed to explain the observations.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
