HE 0017+0055: A probable pulsating CEMP-rs star and long-period binary-Reference-Cited by-同舟云学术

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HE 0017+0055: A probable pulsating CEMP-rs star and long-period binary

Published:2016-02 Issue: Volume:586 Page:A159
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Jorissen A.,Hansen T.,Van Eck S.,Andersen J.,Nordström B.,Siess L.,Torres G.,Masseron T.,Van Winckel H.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201526993/pdf

Reference62 articles.

1. Wind Roche-lobe overflow: Application to carbon-enhanced metal-poor stars

2. Carbon‐enhanced Metal‐poor Stars. I. Chemical Compositions of 26 Stars

3. The Chemical Composition of the Sun

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1. Classification and characterization using HCT/HFOSC spectra of carbon stars selected from the HES survey;Astrophysics and Space Science;2024-01

2. Spectroscopic Study of Four Metal-poor Carbon Stars from the Hamburg/ESO Survey: On Confirming the Low-mass Nature of Their Companions*;The Astrophysical Journal;2022-07-29

3. Observational Evidence Points at AGB Stars as Possible Progenitors of CEMP-s and CEMP-r/s Stars*;The Astrophysical Journal;2021-11-01

4. Optical and NIR spectroscopy of cool CEMP stars to probe the nucleosynthesis in low-mass AGB binary system;Monthly Notices of the Royal Astronomical Society;2021-05-28

5. Spectroscopic study of CEMP-(s & r/s) stars;Astronomy & Astrophysics;2021-05

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