The Open Cluster Chemical Abundances and Mapping Survey. II. Precision Cluster Abundances for APOGEE Using SDSS DR14-Reference-Cited by-同舟云学术

The Open Cluster Chemical Abundances and Mapping Survey. II. Precision Cluster Abundances for APOGEE Using SDSS DR14

Published:2018-09-06 Issue:4 Volume:156 Page:142
ISSN:1538-3881
Container-title:The Astronomical Journal
language:
Short-container-title:AJ

Author:

Donor John,Frinchaboy Peter M.^ORCID,Cunha Katia,Thompson Benjamin,O’Connell Julia^ORCID,Zasowski Gail^ORCID,Jackson Kelly M.,McGrath Brianne Meyer,Almeida Andrés,Bizyaev Dmitry,Carrera Ricardo^ORCID,García-Hernández D. A.,Nitschelm Christian,Pan Kaike^ORCID,Zamora Olga

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/1538-3881/156/i=4/a=142/pdf

Reference76 articles.

1. The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the Extended Baryon Oscillation Spectroscopic Survey and from the Second Phase of the Apache Point Observatory Galactic Evolution Experiment

2. SOUNDING OPEN CLUSTERS: ASTEROSEISMIC CONSTRAINTS FROM KEPLER ON THE PROPERTIES OF NGC 6791 AND NGC 6819

3. Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe

4. Metal Abundances of Red Clump Stars in Open Clusters. I. NGC 6819

Cited by 57 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Exploring fluorine chemical evolution in the Galactic disk: The open cluster perspective;Astronomy & Astrophysics;2024-09

2. Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE;Monthly Notices of the Royal Astronomical Society;2024-08-01

3. A baseline on the relation between chemical patterns and the birth stellar cluster;Astronomy & Astrophysics;2024-08

4. A study on the metallicity gradients in the galactic disk using open clusters;Frontiers in Astronomy and Space Sciences;2024-04-02

5. The GALAH survey: elemental abundances in open clusters using joint effective temperature and surface gravity photometric priors;Monthly Notices of the Royal Astronomical Society;2024-02-13