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dc.contributor.authorGirichidis, Philipp
dc.contributor.authorOffner, Stella S. R.
dc.contributor.authorKritsuk, Alexei G.
dc.contributor.authorKlessen, Ralf S.
dc.contributor.authorHennebelle, Patrick
dc.contributor.authorKruijssen, J. M. Diederik
dc.contributor.authorKrause, Martin G. H.
dc.contributor.authorGlover, Simon C. O.
dc.contributor.authorPadovani, Marco
dc.date.accessioned2020-10-09T00:10:12Z
dc.date.available2020-10-09T00:10:12Z
dc.date.issued2020-06-02
dc.identifier.citationGirichidis , P , Offner , S S R , Kritsuk , A G , Klessen , R S , Hennebelle , P , Kruijssen , J M D , Krause , M G H , Glover , S C O & Padovani , M 2020 , ' Physical Processes in Star Formation ' , Space Science Reviews , vol. 216 , 68 . https://doi.org/10.1007/s11214-020-00693-8
dc.identifier.issn0038-6308
dc.identifier.otherPURE: 21506641
dc.identifier.otherPURE UUID: 5a8d7e2f-1531-4e89-8ed0-028b7087e5dd
dc.identifier.otherArXiv: http://arxiv.org/abs/2005.06472v1
dc.identifier.otherORCID: /0000-0002-9610-5629/work/81741731
dc.identifier.otherScopus: 85085864237
dc.identifier.urihttp://hdl.handle.net/2299/23225
dc.description© 2020 Springer-Verlag. The final publication is available at Springer via https://doi.org/10.1007/s11214-020-00693-8.
dc.description.abstractStar formation is a complex multi-scale phenomenon that is of significant importance for astrophysics in general. Stars and star formation are key pillars in observational astronomy from local star forming regions in the Milky Way up to high-redshift galaxies. From a theoretical perspective, star formation and feedback processes (radiation, winds, and supernovae) play a pivotal role in advancing our understanding of the physical processes at work, both individually and of their interactions. In this review we will give an overview of the main processes that are important for the understanding of star formation. We start with an observationally motivated view on star formation from a global perspective and outline the general paradigm of the life-cycle of molecular clouds, in which star formation is the key process to close the cycle. After that we focus on the thermal and chemical aspects in star forming regions, discuss turbulence and magnetic fields as well as gravitational forces. Finally, we review the most important stellar feedback mechanisms.en
dc.format.extent67
dc.language.isoeng
dc.relation.ispartofSpace Science Reviews
dc.rightsEmbargoed
dc.subjectastro-ph.GA
dc.subjectastro-ph.SR
dc.titlePhysical Processes in Star Formationen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.date.embargoedUntil2021-06-02
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2020-06-02
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1007/s11214-020-00693-8
rioxxterms.licenseref.uriUnspecified
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeEmbargoed


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