This paper covers two subjects in the field of massive star formation which in its details can be discussed separately. Therefore, we present first characteristics of precursors of UCHII regions and their likely evolutionary properties. The second section discusses massive molecular outflows, their implications for high-mass star formation, and a possible evolutionary sequence for massive outflows.
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© 2005 Springer Science+Business Media, Inc
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Beuther, H., Shepherd, D. (2005). Precursors of UchII Regions and the Evolution of Massive Outflows. In: Kumar, M.S.N., Tafalla, M., Caselli, P. (eds) Cores to Clusters. Astrophysics and Space Science Library, vol 324. Springer, New York, NY. https://doi.org/10.1007/0-387-26357-8_8
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DOI: https://doi.org/10.1007/0-387-26357-8_8
Publisher Name: Springer, New York, NY
Print ISBN: 978-0-387-26322-9
Online ISBN: 978-0-387-26357-1
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