Dusty Common Envelope Evolution

We present the first hydrodynamical simulations of common envelope evolution that include the formation of dust and the effect of radiation pressure on dust grains. We performed smoothed particle hydrodynamics simulations of the CE evolution for two systems made of a 1.7 <inline-formula><ma...

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Bibliographic Details
Main Authors: Lionel Siess, Luis C. Bermúdez-Bustamante, Orsola De Marco, Daniel J. Price, Miguel González-Bolívar, Chunliang Mu, Mike Y. M. Lau, Ryosuke Hirai, Taïssa Danilovich
Format: Article
Language:English
Published: MDPI AG 2024-11-01
Series:Galaxies
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Online Access:https://www.mdpi.com/2075-4434/12/6/82
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