Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S315(11), 2015
DOI: 10.1017/s1743921316008139
Full text: Unavailable
AbstractSubmillimetre observations of externally irradiated low-mass protostellar envelopes show that the gas temperature in the envelopes is dominated by the external irradiation. Detailed studies of the protostar IRS7B in Corona Australis also show that the chemistry is strongly affected by the irradiation, depleting the abundances of complex organic molecules.