A multiwavelength study of the star forming region IRAS 18544+0112

Aims: This work aims at investigating the molecular and infrared components in the massive young stellar object (MYSO) candidate IRAS 18544+0112. The purpose is to determine the nature and the origin of this infrared source. Methods: To analyze the molecular gas towards IRAS 18544+0112, we have carr...

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Detalles Bibliográficos
Autores principales:	Ortega, M.E., Paron, S., Cichowolski, S., Rubio, M., Castelletti, G., Dubner, G.
Formato:	JOUR
Materias:	HII regions ISM: molecules Stars: formation Angular resolution Atacama Emission profile H II regions High density Infrared components Infrared emissions Infrared source Ionized gas Molecular analysis Molecular clumps Molecular gas Molecular outflows Multi-wavelength study Near-infrared photometry Non-detection Point sources Public data Spitzer Star-forming region Submillimeters Young stellar objects Ionization of gases Light sources Molecules Stars
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v510_n1_p_Ortega
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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