Gieser, C.; Semenov, D.; Beuther, H.; Ahmadi, A.; Mottram, J. C.; Henning, Th; Beltran, M.; Maud, L. T.; Bosco, F.; Leurini, S.; Peters, T.; Klaassen, P.; Kuiper, R.; Feng, S.; Urquhart, J. S.; Moscadelli, L.; Csengeri, T.; Lumsden, S.; Winters, J. M.; Suri, S.; Zhang, Qizhou; Pudritz, R.; Palau, A.; Menten, K. M.; Galvan-Madrid, R.; Wyrowski, F.; Schilke, P.; Sánchez-Monge, Á.; Linz, H.; Johnston, K. G.; Jiménez-Serra, I.; Longmore, S.; Möller, T.
(2019)
<br/> Aims: In order to understand the observed molecular diversity in high-mass star-forming regions, we have to determine the underlying physical and chemical structure of those regions at high angular resolution and ...