SCHNEIDER, Nicholas; SIMON, Ralph; BONTEMPS, Sylvain; ROY, Arabindo; BONNE, Lars; YAHIA, Hussein; ATTUEL, Guillaume

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Licencia de uso del documento

SCHNEIDER, Nicholas
Laboratory for Atmospheric and Space Physics [Boulder] [LASP]

SIMON, Ralph
Helmholtz zentrum für Schwerionenforschung GmbH [GSI]

BONTEMPS, Sylvain
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]

Idioma

Communication dans un congrès

Este ítem está publicado en

SF2A-2018 - Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: P. Di Matteo, F. Billebaud, F. Herpin, N. Lagarde, J.-B. Marquette, A. Robin, O. Venot, pp.179-180, 2018-07-03, Bordeaux.

Resumen en inglés

The formation of stars is intimately linked to the structure and evolution of molecular clouds in the interstellar medium. The French-German (ANR/DFG) collaborative project GENESIS (GENeration and Evolution of Structures in the ISm, http://www.astro.uni-koeln.de/GENESIS), explores this link with a new approach: by combining far-infrared data of dust (Herschel), observations of major cooling lines in the interstellar medium (CII, CI, CO, OI with the Stratospheric Observatory for FIR astronomy SOFIA), and molecular line maps from ground-based telescopes. It is also supported by the German Government funded MOBS (Modelling SOFIA data). We here present results of two workpackages, one showing SOFIA OI observations in the massive star-forming regions S106, and one investigating molecular cloud formation in the diffuse Draco cloud.< Leer menos

Palabras clave en inglés

PDRs

Star formation

Cloud formation

ISM structure

Orígen

Importado de Hal

Centros de investigación

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804