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What probability distribution functions tell us about the processes of star formation
PERETTO, N.
Département d'Astrophysique (ex SAP) [DAP]
Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
< Reduce
Département d'Astrophysique (ex SAP) [DAP]
Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
Language
en
Communication dans un congrès
This item was published in
proceedings of The 6th Zermatt ISM Symposium: Conditions and Impact of Star Formation, held in Zermatt Switzerlant, 2015, september 7-11, Edited by R. Simon, R. Schaaf and J. Stutzki. EAS Publications Series, Volume 75-76, 2016, pp.175-176, 2015-09-07, Zermatt. 2016, vol. 75-76
English Abstract
Probability distribution functions of column density (N-PDFs) are used to evaluate the relative importance of gravity, turbulence, magnetic fields, geometry, and radiative feedback governing the cloud's density structure ...Read more >
Probability distribution functions of column density (N-PDFs) are used to evaluate the relative importance of gravity, turbulence, magnetic fields, geometry, and radiative feedback governing the cloud's density structure and star-formation activity. These proce- sses influence the N-PDF and thus determine their shape, ranging from a purely lognormal distribution to one with power-law tail(s).Read less <
Origin
Hal imported