Physical properties of the star-forming clusters in NGC 6334

[Aims] We aim to characterise certain physical properties of high-mass star-forming sites in the NGC 6334 molecular cloud, such as the core mass function (CMF), spatial distribution of cores, and mass segregation.

Detalhes bibliográficos
Autores: Sadaghiani, M., Sánchez-Monge, Álvaro, Schilke, Peter, Liu, Hauyu Baobab, Clarke, S. D., Zhang, Qizhou, Girart, Josep Miquel, Seifried, D., Aghababaei, A., Li, Huabai, Juárez, Carmen, Tang, K. S.
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2020
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/233241
Acesso em linha:http://hdl.handle.net/10261/233241
Access Level:acceso abierto
Palavra-chave:ISM: clouds
ISM: individual objects: NGC 6334-I
ISM: individual objects: NGC 6334-I(N)
Stars: massive
Submillimetre: ISM
Stars: formation
Descrição
Resumo:[Aims] We aim to characterise certain physical properties of high-mass star-forming sites in the NGC 6334 molecular cloud, such as the core mass function (CMF), spatial distribution of cores, and mass segregation.

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