Hot Molecular Cores and High-Mass Star Formation

Simple item page
dc.creatorvan der Tak, F. F. S.
dc.date2003-09-04
dc.date.accessioned2026-07-07T02:09:26Z
dc.date.available2026-07-07T02:09:26Z
dc.descriptionThis review covers hot cores in the context of high-mass star formation. After giving an overview of chemical processes and diversity during high-mass star formation, it reviews the `warm envelope' phase which probably precedes the formation of hot cores. Some recent determinations of the cosmic-ray ionization rate are discussed, as well as recent evidence for hot cores around low-mass stars. Routes for future hot core research are outlined.
dc.description8 pages, 1 figure; to appear in the Proceeding of IAU Symposium 221, Star Formation at High Angular Resolution, Editors M. Burton, R. Jayawardhana & T. Bourke, Astronomical Society of the Pacific
dc.identifierhttps://arxiv.org/abs/astro-ph/0309152
dc.identifierhttp://arxiv.org/abs/astro-ph/0309152
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6428
dc.subjectAstrophysics
dc.titleHot Molecular Cores and High-Mass Star Formation
dc.typetext

Files

Collections

arXiv