The Stellar Density in High Mass Star Forming Regions

dc.date.accessioned2020-08-04T21:50:37Z
dc.date.accessioned2022-10-18T23:14:13Z
dc.date.available2020-08-04T21:50:37Z
dc.date.available2022-10-18T23:14:13Z
dc.date.created2020-08-04T21:50:37Z
dc.date.issued2003
dc.identifierhttp://hdl.handle.net/10533/242412
dc.identifier15010003
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4473702
dc.description.abstractRecent theoretical work has suggested that massive stars may form through the collisional agglomeration of lower mass stars in the dense centers of young stellar clusters. Densities in excess of 100 million stars per cubic parsec are required for collisio
dc.languageeng
dc.publisherSydney
dc.relationhttps://ui.adsabs.harvard.edu/abs/2003IAUS..221P.209M/abstract
dc.relationinstname: ANID
dc.relationreponame: Repositorio Digital RI2.0
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleThe Stellar Density in High Mass Star Forming Regions
dc.typeCapitulo de libro


Este ítem pertenece a la siguiente institución