Variability in the Massive Open Cluster NGC 1817 from K2: A Rich Population of Asteroseismic Red Clump, Eclipsing Binary, and Main-sequence Pulsating Stars-Reference-Cited by-同舟云学术

Variability in the Massive Open Cluster NGC 1817 from K2: A Rich Population of Asteroseismic Red Clump, Eclipsing Binary, and Main-sequence Pulsating Stars

Published:2020-02-10 Issue:3 Volume:159 Page:96
ISSN:1538-3881
Container-title:The Astronomical Journal
language:
Short-container-title:AJ

Author:

Sandquist Eric L.^ORCID,Stello Dennis^ORCID,Arentoft Torben^ORCID,Brogaard Karsten^ORCID,Grundahl Frank^ORCID,Vanderburg Andrew^ORCID,Hedlund Anne^ORCID,DeWitt Ryan,Ackerman Taylor R.,Aguilar Miguel,Buckner Andrew J.^ORCID,Juarez Christian,Ortiz Arturo J.,Richarte David,Rivera Daniel I.,Schlapfer Levi

Funder

NASA

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-3881/ab68df/pdf

Reference86 articles.

1. A Dozen δ Scuti Stars in the Open Cluster NGC 1817

2. Convective-core Overshoot and Suppression of Oscillations: Constraints from Red Giants in NGC 6811

3. Chemical composition of giant stars in the open cluster IC 4756

4. uvby–H$_{\beta}$ CCD photometry of NGC 1817 and NGC 1807

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