Exploring the 13CO/C18O abundance ratio towards Galactic young stellar objects and H II regions

Aims. Determining molecular abundance ratios is important not only for the study of Galactic chemistry, but also because they are useful to estimate physical parameters in a large variety of interstellar medium environments. One of the most important molecules for tracing the molecular gas in the in...

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Detalles Bibliográficos
Publicado:	2018
Materias:	Galaxy: abundances HII regions ISM: abundances ISM: molecules Stars: formation Galaxies Isotopes Stars Surveys H II regions ISM: abundance Molecules
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v612_n_p_Areal http://hdl.handle.net/20.500.12110/paper_00046361_v612_n_p_Areal
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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