Modelling the abundance structure of isocyanic acid (HNCO) towards the low-mass 
solar type protostar IRAS 16293-2422

Hernández-Gómez, A.; Sahnoun, E.; Caux, E.; Wiesenfeld, L.; Loinard, L.; Bottinelli, S.; Hammami, K.; Menten, K.M.

doi:10.1093/mnras/sty2971

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Modelling the abundance structure of isocyanic acid (HNCO) towards the low-mass solar type protostar IRAS 16293-2422

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Menten, K.M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Hernández-Gómez, A., Sahnoun, E., Caux, E., Wiesenfeld, L., Loinard, L., Bottinelli, S., et al. (2019). Modelling the abundance structure of isocyanic acid (HNCO) towards the low-mass solar type protostar IRAS 16293-2422. mnras, 483(2), 2014-2030. doi:10.1093/mnras/sty2971.

Cite as: https://hdl.handle.net/21.11116/0000-0006-7A27-6

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