2004/04/28 by H. Beuther, Beuther, H.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0404563
8 pages, 4 figures, conference proceedings (invited talk) of the "X-ray and Radio Connections" meeting in Santa Fe in February 2004
arxiv created 2004/04/28 · arxiv updated 2009/12/01
Studying outflows from young massive star-forming clusters allows one to deduce physical processes that lead to the formation of the most massive stars. I will review the current state of high-spatial-resolution interferometric (sub-)mm studies of massive molecular outflows and their implications for high-mass star formation. A possible evolutionary scenario for massive outflows with highly collimated structures at the very beginning and more wind-like outflows at later stages will be outlined.