Triggering star formation : experimental compression of a foam ball induced by Taylor-Sedov blast waves

The interaction between a molecular cloud and an external agent (e.g., a supernova remnant, plasma jet, radiation, or another cloud) is a common phenomenon throughout the Universe and can significantly change the star formation rate within a galaxy. This process leads to fragmentation of the cloud a...

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Main Authors: Albertazzi, B, Mabey, P, Michel, Th, Meinecke, J, Gregori, G
Format: Journal article
Language:English
Published: AIP Publishing 2022
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author Albertazzi, B
Mabey, P
Michel, Th
Meinecke, J
Gregori, G
author_facet Albertazzi, B
Mabey, P
Michel, Th
Meinecke, J
Gregori, G
author_sort Albertazzi, B
collection OXFORD
description The interaction between a molecular cloud and an external agent (e.g., a supernova remnant, plasma jet, radiation, or another cloud) is a common phenomenon throughout the Universe and can significantly change the star formation rate within a galaxy. This process leads to fragmentation of the cloud and to its subsequent compression and can, eventually, initiate the gravitational collapse of a stable molecular cloud. It is, however, difficult to study such systems in detail using conventional techniques (numerical simulations and astronomical observations), since complex interactions of flows occur. In this paper, we experimentally investigate the compression of a foam ball by Taylor–Sedov blast waves, as an analog of supernova remnants interacting with a molecular cloud. The formation of a compression wave is observed in the foam ball, indicating the importance of such experiments for understanding how star formation is triggered by external agents.
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spelling oxford-uuid:abc514b7-df71-4e6f-8aa7-db33e02501b22022-05-24T15:15:20ZTriggering star formation : experimental compression of a foam ball induced by Taylor-Sedov blast wavesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:abc514b7-df71-4e6f-8aa7-db33e02501b2EnglishSymplectic ElementsAIP Publishing2022Albertazzi, BMabey, PMichel, ThMeinecke, JGregori, GThe interaction between a molecular cloud and an external agent (e.g., a supernova remnant, plasma jet, radiation, or another cloud) is a common phenomenon throughout the Universe and can significantly change the star formation rate within a galaxy. This process leads to fragmentation of the cloud and to its subsequent compression and can, eventually, initiate the gravitational collapse of a stable molecular cloud. It is, however, difficult to study such systems in detail using conventional techniques (numerical simulations and astronomical observations), since complex interactions of flows occur. In this paper, we experimentally investigate the compression of a foam ball by Taylor–Sedov blast waves, as an analog of supernova remnants interacting with a molecular cloud. The formation of a compression wave is observed in the foam ball, indicating the importance of such experiments for understanding how star formation is triggered by external agents.
spellingShingle Albertazzi, B
Mabey, P
Michel, Th
Meinecke, J
Gregori, G
Triggering star formation : experimental compression of a foam ball induced by Taylor-Sedov blast waves
title Triggering star formation : experimental compression of a foam ball induced by Taylor-Sedov blast waves
title_full Triggering star formation : experimental compression of a foam ball induced by Taylor-Sedov blast waves
title_fullStr Triggering star formation : experimental compression of a foam ball induced by Taylor-Sedov blast waves
title_full_unstemmed Triggering star formation : experimental compression of a foam ball induced by Taylor-Sedov blast waves
title_short Triggering star formation : experimental compression of a foam ball induced by Taylor-Sedov blast waves
title_sort triggering star formation experimental compression of a foam ball induced by taylor sedov blast waves
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