LOW-RESOLUTION SPECTROSCOPY FOR THE GLOBULAR CLUSTERS WITH SIGNS OF SUPERNOVA ENRICHMENT: M22, NGC 1851, AND NGC 288-Reference-Cited by-同舟云学术

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LOW-RESOLUTION SPECTROSCOPY FOR THE GLOBULAR CLUSTERS WITH SIGNS OF SUPERNOVA ENRICHMENT: M22, NGC 1851, AND NGC 288

Published:2015-01-14 Issue:1 Volume:216 Page:19
ISSN:1538-4365
Container-title:The Astrophysical Journal Supplement Series
language:
Short-container-title:ApJS

Author:

Lim Dongwook,Han Sang-Il,Lee Young-Wook,Roh Dong-Goo,Sohn Young-Jong,Chun Sang-Hyun,Lee Jae-Woo,Johnson Christian I.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.1088/0067-0049/216/1/19/pdf

Reference94 articles.

1. MIXED POPULATIONS IN GLOBULAR CLUSTERS: ET TU, 47 TUC?

2. uvbyCaH CCD Photometry of Clusters. IV. Solving the Riddle of NGC 3680

3. CN and CA abundance variations among the giants in M22

4. CA II H and K filter photometry on the UVBY system. I - The standard system

5. The influence of residual gas expulsion on the evolution of the Galactic globular cluster system and the origin of the Population II halo

Cited by 35 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. The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios;Monthly Notices of the Royal Astronomical Society;2023-10-03

2. Blanco DECam Bulge Survey (BDBS). VI. Extinction Maps Toward Southern Galactic Bulge Globular Clusters;The Astrophysical Journal;2023-06-01

3. Peeking beneath the precision floor – I. Metallicity spreads and multiple elemental dispersions in the globular clusters NGC 288 and NGC 362;Monthly Notices of the Royal Astronomical Society;2022-10-22

4. The complex stellar system M 22: confirming abundance variations with high precision differential measurements;Monthly Notices of the Royal Astronomical Society;2022-08-13

5. HST Observations of the Globular Cluster NGC 6402 (M14) and Its Peculiar Multiple Populations;The Astrophysical Journal;2022-02-01

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