Search for filamentary accretion through low velocity shocks
| Autor: | Bonne , Lars, Bontemps , sylvain, Schneider , Nicola, Csengeri , Timea, Yahia , Hussein, Güsten , Rolf, Attuel , Guillaume, Roy , Arabindo, Simon , Robert |
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| Přispěvatelé: | Laboratoire d'Astrophysique de Bordeaux [Pessac] ( LAB ), Université de Bordeaux ( UB ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), I. Physikalisches Institut [Köln], Universität zu Köln, Max-Planck-Institut für Radioastronomie ( MPIFR ), Geometry and Statistics in acquisition data ( GeoStat ), Inria Bordeaux - Sud-Ouest, Institut National de Recherche en Informatique et en Automatique ( Inria ) -Institut National de Recherche en Informatique et en Automatique ( Inria ), Supported by Deutsche Forschungsgemeinde (DFG) and the Agence nationale de recherche (ANR). GENeration and Evolution of Structures in the ISm. Duration: start 1.5. 2017, 3 years. Coordinator: N. Schneider (I. Physik, Cologne)., GENeration and Evolution of Structures in the ISm (GENESIS), Yahia, H., Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Formation Stellaire, Universität zu Köln = University of Cologne, Max-Planck-Institut für Radioastronomie (MPIFR), Geometry and Statistics in acquisition data (GeoStat), Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria) |
| Jazyk: | angličtina |
| Rok vydání: | 2018 |
| Předmět: |
[ INFO.INFO-TS ] Computer Science [cs]/Signal and Image Processing
[INFO.INFO-TS] Computer Science [cs]/Signal and Image Processing Astrophysics::High Energy Astrophysical Phenomena [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph] [PHYS.ASTR.GA] Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] Astrophysics::Cosmology and Extragalactic Astrophysics [PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] [INFO.INFO-TS]Computer Science [cs]/Signal and Image Processing [ PHYS.ASTR.GA ] Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] Astrophysics::Solar and Stellar Astrophysics ComputingMethodologies_GENERAL [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph] Astrophysics::Galaxy Astrophysics |
| Zdroj: | Science with the ATACAMA Pathfinder Experiment (APEX) Science with the ATACAMA Pathfinder Experiment (APEX), Mar 2018, Schloss Ringberg, Germany. 2018, 〈https://events.mpifr-bonn.mpg.de/indico/event/58/overview〉 |
| Popis: | International audience; Filamentary star formation Herschel observations revealed the ubiquitous presence of interstellar filaments and their importance in star formation (e.g. [1],[2],[3]). It is proposed that they form by dissipation of kinetic energy in large scale magneto-hydrodynamic flows through low-velocity magnetised shocks (C-shocks) and then fragment in prestellar cores after reaching a density threshold of ∼ 16 M /pc [4],[5]. There are indications that these filaments accrete mass through inflow of matter from the sides along the magnetic field (e.g. [6],[7]). However, direct evidence of such shocks is vital to confirm this scenario. |
| Databáze: | OpenAIRE |
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