Ionization compression impact on dense gas distribution and star formation
2014; EDP Sciences; Volume: 564; Linguagem: Inglês
10.1051/0004-6361/201322700
ISSN1432-0746
AutoresPascal Tremblin, N. Schneider, V. Minier, P. Didelon, T. Hill, L. D. Anderson, F. Motte, A. Zavagno, Ph. André, D. Arzoumanian, E. Audit, M. Benedettini, S. Bontemps, T. Csengeri, James Di Francesco, T. Giannini, M. Hennemann, Q. Nguyễn Lương, A. P. Marston, N. Peretto, A. Rivera-Ingraham, D. Russeil, K. L. J. Rygl, L. Spinoglio, G. J. White,
Tópico(s)Galaxies: Formation, Evolution, Phenomena
ResumoAims. Ionization feedback should impact the probability distribution function (PDF) of the column density of cold dust around the ionized gas. We aim to quantify this effect and discuss its potential link to the core and initial mass function (CMF/IMF).
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