The Gaia-ESO Survey: membership and initial mass function of the γ Velorum cluster

Context. Understanding the properties of young open clusters, such as the initial mass function (IMF), star formation history, and dynamic evolution, is crucial for obtaining reliable theoretical predictions of the mechanisms involved in the star formation process.

Detalles Bibliográficos
Autores: Prisinzano, L., Damiani, F., Micela, G., Jeffries, R. D., Franciosini, E., Sacco, G. G., Frasca, A., Klutsch, A., Lanzafame, A., Alfaro, Emilio J., Biazzo, K., Bonito, R., Bragaglia, A., Caramazza, M., Vallenari, A., Carraro, G., Costado, M. T., Flaccomio, E., Jofré, P., Lardo, C., Monaco, L., Morbidelli, L., Mowlavi, N., Pancino, E., Randich, S., Zaggia, S.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2016
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/395578
Acceso en línea:http://hdl.handle.net/10261/395578
Access Level:acceso abierto
Palabra clave:Stars: pre-main sequence
Open clusters and associations: individual: γVelorum
Stars: formation
Stars: luminosity function, mass function
Techniques: radial velocities
Techniques: spectroscopic
Descripción
Sumario:Context. Understanding the properties of young open clusters, such as the initial mass function (IMF), star formation history, and dynamic evolution, is crucial for obtaining reliable theoretical predictions of the mechanisms involved in the star formation process.

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