What probability distribution functions tell us about the processes of star formation
| hal.structure.identifier | DAM Île-de-France [DAM/DIF] | |
| dc.contributor.author | SCHNEIDER, N. | |
| hal.structure.identifier | DAM Île-de-France [DAM/DIF] | |
| dc.contributor.author | OSSENKOPF, V. | |
| hal.structure.identifier | Universität Heidelberg [Heidelberg] = Heidelberg University | |
| dc.contributor.author | KLESSEN, R.S. | |
| hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
| dc.contributor.author | CSENGERI, T. | |
| hal.structure.identifier | Materialprüfungsanstalt Universität Stuttgart [Stuttgart] [MPA] | |
| dc.contributor.author | GIRICHIDIS, P. | |
| hal.structure.identifier | University of Canberra | |
| dc.contributor.author | FEDERRATH, C. | |
| hal.structure.identifier | Maison de la Simulation [MDLS] | |
| hal.structure.identifier | University of Exeter | |
| dc.contributor.author | TREMBLIN, Pascal | |
| hal.structure.identifier | FORMATION STELLAIRE 2016 | |
| dc.contributor.author | BONTEMPS, Sylvain | |
| hal.structure.identifier | Département d'Astrophysique (ex SAP) [DAP] | |
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | PERETTO, N. | |
| hal.structure.identifier | DAM Île-de-France [DAM/DIF] | |
| dc.contributor.author | SIMON, R. | |
| hal.structure.identifier | Physikalisches Institut [Köln] | |
| dc.contributor.author | STUTZKI, J. | |
| dc.date.issued | 2016 | |
| dc.date.conference | 2015-09-07 | |
| dc.description.abstractEn | 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). | |
| dc.language.iso | en | |
| dc.title.en | What probability distribution functions tell us about the processes of star formation | |
| dc.type | Communication dans un congrès | |
| dc.identifier.doi | 10.1051/eas/1575031 | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA] | |
| bordeaux.volume | 75-76 | |
| bordeaux.conference.title | 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 | |
| bordeaux.country | CH | |
| bordeaux.conference.city | Zermatt | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | hal-01323797 | |
| hal.version | 1 | |
| hal.invited | non | |
| hal.proceedings | non | |
| hal.conference.end | 2015-09-11 | |
| hal.popular | non | |
| hal.audience | Internationale | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-01323797v1 | |
| bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2016&rft.volume=75-76&rft.au=SCHNEIDER,%20N.&OSSENKOPF,%20V.&KLESSEN,%20R.S.&CSENGERI,%20T.&GIRICHIDIS,%20P.&rft.genre=unknown |
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