The molecular gas around the luminous blue variable star G24.73+0.69

Aims. We study the molecular environment of the luminous blue variable star G24.73+0.69 to investigate the origin of the two infrared shells around this massive star and determine its effects on the surrounding interstellar medium. Methods. We analyze the distribution of the molecular gas using the...

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Detalles Bibliográficos
Autores principales:	Petriella, A., Paron, S.A., Giacani, E.B.
Formato:	JOUR
Materias:	ISM: clouds stars: formation stars: individual: G24.73+0.69 stars: winds, outflows Interstellar mediums ISM : clouds Luminous Blue Variables Massive stars Midinfrared Molecular environment Molecular gas Molecular materials Stars: individual Stellar wind Supernova remnants Young stellar objects Luminance Molecules Shells (structures) Stars
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v538_n_p_Petriella
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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