The Impact of Outflows: From Low to High Mass Protostars
Language
en
Communication dans un congrès
This item was published in
Astrophysics and Space Science Proceedings, 2014ASSP...36..407D - The Labyrinth of Star Formation, held in Greece, june 2012, Astrophysics and Space Science Proceedings, Volume 36. ISBN 978-3-319-03040-1. Springer International Publishing Switzerland, p. 407, 2014, 2014ASSP...36..407D - The Labyrinth of Star Formation, held in Greece, june 2012, Astrophysics and Space Science Proceedings, Volume 36. ISBN 978-3-319-03040-1. Springer International Publishing Switzerland, p. 407, 2014, 2012. 2014, vol. 36, p. 407
Springer
English Abstract
Despite the importance of outflows in removing angular momentum and mass from protostellar envelopes, we struggle to understand their origin, their changes with mass and evolutionary stage of the protostars, and their ...Read more >
Despite the importance of outflows in removing angular momentum and mass from protostellar envelopes, we struggle to understand their origin, their changes with mass and evolutionary stage of the protostars, and their impact on the dynamics of proto-clusters. Here we present our recent observational work addressing these issues, including the study of a low mass star forming region (B59), with a direct measurement of the outflows impact and turbulence injection; and a test of low mass evolutionary models on a sample of high mass protostars in Cygnus X.Read less <
English Keywords
Physics
Origin
Hal imported