Radio observations of the isotopic composition of the galaxy

Details Radio observations of the isotopic composition of the galaxy Radio observations of the isotopic composition of the galaxy

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..402..265b&link_type=abstract

Astrophysical implications of the laboratory study of presolar materials. AIP Conference Proceedings, Volume 402, pp. 265-283 (

Astronomy and Astrophysics

Astrophysics

3

Chemical Composition And Chemical Evolution, Interstellar Medium And Nebulae In Milky Way, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Radio, Microwave

Scientific paper

The determination of elemental isotope abundances in the Galaxy through the use of radio-frequency molecular lines is reviewed. Advantages and potential sources of systematic error are summarized. Results for the gas in the Galactic disk molecular clouds, and for the circumstellar envelopes of cool evolved stars are given, with emphasis on recent results. Some implications for models of nucleosynthesis and galactic chemical evolution are noted.

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