Type II Cepheids: evidence for Na–O anticorrelation for BL Her type stars?-Reference-Cited by-同舟云学术

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Type II Cepheids: evidence for Na–O anticorrelation for BL Her type stars?

Published:2018-03-14 Issue:2 Volume:477 Page:2276-2285
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Kovtyukh V¹²,Yegorova I³,Andrievsky S¹²⁴,Korotin S¹⁵,Saviane I⁶,Lemasle B⁷,Chekhonadskikh F¹²,Belik S¹²

Affiliation:

1. Astronomical Observatory, Odessa National University, Shevchenko Park, UA-65014 Odessa, Ukraine

2. Isaac Newton Institute of Chile, Odessa branch, Shevchenko Park, UA-65014 Odessa, Ukraine

3. Universidad Andres Bello, Fernandez Concha 700, Santiago, Chile

4. GEPI, Observatoire de Paris-Meudon, CNRS, Universite Paris Diderot, F-92125 Meudon Cedex, France

5. Crimean Astrophysical Observatory, Nauchny UA-298409, Crimea, Ukraine

6. European Southern Observatory, Alonso de Cordova 3107, Santiago, Chile

7. Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12-14, D-69120 Heidelberg, Germany

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/477/2/2276/25009584/sty671.pdf

Reference58 articles.

1. Towards the solution of the Bootis problem

2. KP Cyg: An Unusual Metal-Rich RR Lyr Type Star of Long Period

3. $\mathsf{\alpha}$-, r-, and s-process element trends in the Galactic thin and thick disks

4. Exploring the Milky Way stellar disk

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