Chemical composition of post-AGB star candidates-Reference-Cited by-同舟云学术

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Chemical composition of post-AGB star candidates

Published:2018-11 Issue:9-10 Volume:339 Page:680-697
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron. Nachr.

Author:

Molina R. E.¹,Pereira C. B.²,Arellano Ferro A.³

Affiliation:

1. Laboratorio de Investigación en Física Aplicada y Computacional; Universidad Nacional Experimental del Táchira; San Cristóbal Venezuela

2. Observatório Nacional/MCTI; Rio de Janeiro Brazil

3. Instituto de Astronomía; Universidad Nacional Autónoma de México; Ciudad de México Mexico

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/asna.201913542/fullpdf

Reference100 articles.

1. The optically bright post-AGB population of the LMC

2. Detailed abundance study of four s-process enriched post-AGB stars in the Large Magellanic Cloud

3. Atmospheric abundances in post-AGB candidates of intermediate temperature

4. Photometric variability of five candidates for protoplanetary nebulae

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