Mean density inversions for red giants and red clump stars-Reference-Cited by-同舟云学术

Mean density inversions for red giants and red clump stars

Published:2018-08-27 Issue:2 Volume:482 Page:2305-2319
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Buldgen Gaël¹,Rendle B¹,Sonoi T²³,Davies G R¹,Miglio A¹,Salmon S J A J⁴,Reese D R³^ORCID,Bossini D⁵,Eggenberger P⁶,Noels A³,Scuflaire R³

Affiliation:

1. School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK

2. Astronomical Institute, Tohoku University, 6-3 Aramaki Aza-Aoba, Aoba-ku, Sendai 980-8578, Japan

3. LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, F-92195 Meudon, France

4. STAR Institute, Université de Liège, Allée du Six Août 19C, B-4000 Liège, Belgium

5. Observatory of Padua-INAF, Vicolo dell’Osservatorio 5, I-35122 Padova, Italy

6. Observatoire de Genève, Université de Genève, 51 Ch. Des Maillettes, CH-1290 Sauverny, Switzerland

Funder

H2020 European Research Council

Science and Technology Facilities Council

Division of Arctic Sciences

Japan Society for the Promotion of Science

European Commission

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/482/2/2305/26576165/sty2346.pdf

Reference68 articles.

1. Solar fusion cross sections. II. Theppchain and CNO cycles

2. Galactic archaeology with asteroseismology and spectroscopy: Red giants observed by CoRoT and APOGEE

3. Red giants observed by CoRoT and APOGEE: The evolution of the Milky Way’s radial metallicity gradient

4. The Chemical Composition of the Sun

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