Pismis 24-1: The stellar upper mass limit preserved

Is there a stellar upper mass limit? Recent statistical work seems to indicate that there is and that it is in the vicinity of 150 M⊙. In this paper we use HST and ground-based data to investigate the brightest members of the cluster Pismis 24, one of which (Pismis 24-1) was previously inferred to h...

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Detalles Bibliográficos
Autores principales:	Maíz Apellániz, Jesús, Walborn, Nolan Revere, Morrell, Nidia Irene, Niemelä, Virpi Sinikka, Nelan, E. P.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2007
Materias:	Ciencias Astronómicas Binaries: close Stars: early-type Stars: Fundamental parameters Stars: individual (Pismis 24-17, Pismis 24-1NW, Pismis 24-1SE)
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/83142
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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