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  Outflows from the youngest stars are mostly molecular

Ray, T. P., McCaughrean, M. J., Garatti, A. C. o., Kavanagh, P. J., Justtanont, K., van Dishoeck, E. F., et al. (2024). Outflows from the youngest stars are mostly molecular. Nature, 622, 48-52. doi:10.1038/s41586-023-06551-1.

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 Creators:
Ray, T. P., Author
McCaughrean, M. J., Author
Garatti, A. Caratti o, Author
Kavanagh, P. J., Author
Justtanont, K., Author
van Dishoeck, E. F., Author
Reitsma, M., Author
Beuther, H., Author
Francis, L., Author
Gieser, C.1, Author           
Klaassen, P., Author
Perotti, G., Author
Tychoniec, L., Author
van Gelder, M., Author
Colina, L., Author
Greve, Th. R., Author
Güdel, M., Author
Henning, Th., Author
Lagage, P. O., Author
Östlin, G., Author
Vandenbussche, B., AuthorWright, C. Waelkens G., Author more..
Affiliations:
1Center for Astrochemical Studies at MPE, MPI for Extraterrestrial Physics, Max Planck Society, ou_1950287              

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Language(s): eng - English
 Dates: 2024-08-24
 Publication Status: Published online
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: DOI: 10.1038/s41586-023-06551-1
 Degree: -

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Title: Nature
  Abbreviation : Nature
Source Genre: Journal
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Publ. Info: London : Nature Publishing Group
Pages: - Volume / Issue: 622 Sequence Number: - Start / End Page: 48 - 52 Identifier: ISSN: 0028-0836
CoNE: https://pure.mpg.de/cone/journals/resource/954925427238