Chemical evolution of fluorine in the bulge-Reference-Cited by-同舟云学术

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Chemical evolution of fluorine in the bulge

Published:2014-04 Issue: Volume:564 Page:A122
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Jönsson H.,Ryde N.,Harper G. M.,Cunha K.,Schultheis M.,Eriksson K.,Kobayashi C.,Smith V. V.,Zoccali M.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201423597/pdf

Reference71 articles.

1. FLUORINE IN ASYMPTOTIC GIANT BRANCH CARBON STARS REVISITED

2. THE FIRST FLUORINE ABUNDANCE DETERMINATIONS IN EXTRAGALACTIC ASYMPTOTIC GIANT BRANCH CARBON STARS

3. Chemical similarities between Galactic bulge and local thick disk red giants: O, Na, Mg, Al, Si, Ca, and Ti

4. Abundances of the elements: Meteoritic and solar

5. Vibration–rotational Einstein coefficients for HF/DF and HCl/DCl

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