Induced star formation in the HII region SH2-54

We present a multiwavelength study of the interstellar medium around the HII region Sh2-54. The millimetric and infrared data allow us to analyze and characterize the molecular gas and dust components, respectively. The emision at 8.0 μm of Spitzer-IRAC shows a complex filamentary structure of photo...

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Detalles Bibliográficos
Autores principales:	Vasquez, J., Cappa, C.E., Cichowolski, S., Ortega, M., Romero, G., Rubio, M.
Formato:	CONF
Materias:	HII regions ISM: Individual (Sh2-54) Stars: Formation
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_14052059_v40_n_p259_Vasquez
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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