A molecular outflow revealing star formation activity in the vicinity of the HII region G034.8-0.7 and the SNR W44

Aims. This work aims at investigating the molecular gas component in the vicinity of two young stellar object (YSO) candidates identified at the border of the HII region G034.8-0.7 that is evolving within a molecular cloud shocked by the SNR W44. The purpose is to explore signatures of star forming...

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Detalles Bibliográficos
Autores principales:	Paron, S., Ortega, M.E., Rubio, M., Dubner, G.
Formato:	JOUR
Materias:	ISM: clouds ISM: jets and outflows ISM: molecules Stars: formation Angular resolution Atacama H II regions High density Line of Sight Midinfrared Molecular clouds Molecular gas Molecular outflows Star formations Submillimeter Young stellar objects Acoustic intensity Clouds Molecules Stars Signal to noise ratio
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v498_n2_p445_Paron
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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