Mapping the 13CO/C18O abundance ratio in the massive star-forming region G29.96-0.02

Aims. Estimating molecular abundances ratios from directly measuring the emission of the molecules toward a variety of interstellar environments is indeed very useful to advance our understanding of the chemical evolution of the Galaxy, and hence of the physical processes related to the chemistry. I...

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Detalles Bibliográficos
Autores principales:	Paron, S., Areal, M.B., Ortega, M.E.
Formato:	JOUR
Materias:	Galaxy: abundances HII regions ISM: abundances ISM: molecules Stars: formation Galaxies Giant stars Molecules Surveys H II regions ISM: abundance Ionization of gases
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v617_n_p_Paron
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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