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The winds from HL Tau

Outflowing motions, whether a wind launched from the disc, a jet launched from the protostar, or the entrained molecular outflow, appear to be a ubiquitous feature of star formation. These outwards motions have a number of root causes, and how they manifest is intricately linked to their environment...

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Detalhes bibliográficos
Publicado no:Mon Not R Astron Soc
Main Authors: Klaassen, P. D., Mottram, J. C., Maud, L. T., Juhasz, A.
Formato: Artigo
Idioma:Inglês
Publicado em: Oxford University Press 2016
Assuntos:
Acesso em linha:https://ncbi.nlm.nih.gov/pmc/articles/PMC4985972/
https://ncbi.nlm.nih.gov/pubmed/27559304
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1093/mnras/stw989
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