Chemical complexity in high-mass star formation. An observational and modeling 
case study of the AFGL 2591 VLA 3 hot core

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, Q.; 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.

doi:10.1051/0004-6361/201935865

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Chemical complexity in high-mass star formation. An observational and modeling case study of the AFGL 2591 VLA 3 hot core

MPS-Authors

Csengeri, T.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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

Wyrowski, F.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Gieser, C., Semenov, D., Beuther, H., Ahmadi, A., Mottram, J., Henning, T., et al. (2019). Chemical complexity in high-mass star formation. An observational and modeling case study of the AFGL 2591 VLA 3 hot core. aap, 631: A142, pp. A142. doi:10.1051/0004-6361/201935865.

Cite as: https://hdl.handle.net/21.11116/0000-0006-7F07-5

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