Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback

The physics of star formation and the deposition of mass, momentum, and energy into the interstellar medium by massive stars (‘feedback’) are the main uncertainties in modern cosmological simulations of galaxy formation and evolution1, 2. These processes determine the properties of galaxies3, 4, but...

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Detalles Bibliográficos
Autores principales: Kruijssen, J. M. Diederik, Schruba, Andreas, Chevance, Mélanie, Longmore, Steven N., Hygate, Alexander P. S., Haydon, Daniel T., McLeod, Anna F., Dalcanton, Julianne J., Tacconi, Linda J., van Dishoeck, Ewine F.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: 2019
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6544524/
https://www.ncbi.nlm.nih.gov/pubmed/31118525
http://dx.doi.org/10.1038/s41586-019-1194-3

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6544524/
https://www.ncbi.nlm.nih.gov/pubmed/31118525
http://dx.doi.org/10.1038/s41586-019-1194-3

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