What probability distribution functions tell us about the processes of star formation
Langue
en
Communication dans un congrès
Ce document a été publié dans
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
Résumé en anglais
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 ...Lire la suite >