Molecular gas and star formation toward the IR dust bubble S 24 and its environs

Aims. We present a multiwavelength analysis of the infrared dust bubble S 24 and the extended IR sources G341.220-0.213 and G341.217-0.237 located in its environs. We aim to investigate the characteristics of the molecular gas and the interstellar dust linked to them and analyze the evolutionary sta...

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Detalles Bibliográficos
Autores principales:	Cappa, Cristina Elisabet, Duronea, Nicolás Urbano, Firpo, Verónica, Vasquez, Javier, López Caraballo, C. E., Rubio, Mónica, Vazzano, María Mercedes
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2016
Materias:	Ciencias Astronómicas Hii regions ISM: molecules Molecular data Submillimeter: ISM
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/86096
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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