Author Correction: Outflows from the youngest stars are mostly molecular

T. P. Ray (), M. J. McCaughrean, A. Caratti o Garatti, P. J. Kavanagh, K. Justtanont, E. F. Dishoeck, M. Reitsma, H. Beuther, L. Francis, C. Gieser, P. Klaassen, G. Perotti, L. Tychoniec, M. Gelder, L. Colina, Th. R. Greve, M. Güdel, Th. Henning, P. O. Lagage, G. Östlin, B. Vandenbussche, C. Waelkens and G. Wright
Additional contact information
T. P. Ray: Dublin Institute for Advanced Studies
M. J. McCaughrean: European Space Agency, ESTEC
A. Caratti o Garatti: INAF - Osservatorio Astronomico di Capodimonte
P. J. Kavanagh: Dublin Institute for Advanced Studies
K. Justtanont: Chalmers University of Technology, Onsala Space Observatory
E. F. Dishoeck: Leiden University
M. Reitsma: European Space Agency, ESTEC
H. Beuther: Max-Planck-Institut für Astronomie (MPIA)
L. Francis: Leiden University
C. Gieser: Max-Planck-Institut für Extraterrestrische Physik
P. Klaassen: Royal Observatory Edinburgh
G. Perotti: Max-Planck-Institut für Astronomie (MPIA)
L. Tychoniec: European Southern Observatory
M. Gelder: Leiden University
L. Colina: Centro de Astrobiología (CAB, CSIC-INTA), Carretera de Ajalvir
Th. R. Greve: Technical University of Denmark
M. Güdel: Max-Planck-Institut für Astronomie (MPIA)
Th. Henning: Max-Planck-Institut für Astronomie (MPIA)
P. O. Lagage: Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM
G. Östlin: Stockholm University, AlbaNova University Center
B. Vandenbussche: KU Leuven
C. Waelkens: KU Leuven
G. Wright: Royal Observatory Edinburgh

Nature, 2023, vol. 623, issue 7985, E3-E3

Date: 2023
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DOI: 10.1038/s41586-023-06744-8

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