Outflows from the youngest stars are mostly molecular

The formation of stars and planets is accompanied not only by the build-up of matter, namely accretion, but also by its expulsion in the form of highly supersonic jets that can stretch for several parsecs(1,2). As accretion and jet activity are correlated and because young stars acquire most of thei...

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Detalles Bibliográficos
Autores principales: Ray, T. P., McCaughrean, M. J., Caratti o Garatti, A., Kavanagh, P. J., Justtanont, K., van Dishoeck, E. F., Reitsma, M., Beuther, H., Francis, L., Gieser, C., Klaassen, P., Perotti, G., Tychoniec, L., van Gelder, M., Colina, L., Greve, Th. R., Güdel, M., Henning, Th., Lagage, P. O., Östlin, G., Vandenbussche, B., Waelkens, C., Wright, G.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2023
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10550818/
https://www.ncbi.nlm.nih.gov/pubmed/37619607
http://dx.doi.org/10.1038/s41586-023-06551-1

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10550818/
https://www.ncbi.nlm.nih.gov/pubmed/37619607
http://dx.doi.org/10.1038/s41586-023-06551-1

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