Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – II. Relative ages and distances for six ancient globular clusters-Reference-Cited by-同舟云学术

Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – II. Relative ages and distances for six ancient globular clusters

Published:2017-07-06 Issue:3 Volume:471 Page:3347-3358
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Wagner-Kaiser R.¹,Mackey Dougal²,Sarajedini Ata¹³,Chaboyer Brian⁴,Cohen Roger E.⁵,Yang Soung-Chul⁶,Cummings Jeffrey D.⁷,Geisler Doug⁸,Grocholski Aaron J.⁹

Affiliation:

1. Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611, USA

2. Research School of Astronomy & Astrophysics, Australian National University, Canberra, ACT 2611, Australia

3. Department of Physics, Florida Atlantic University, 777 Glades Rd, Boca Raton, FL 33431, USA

4. Department of Physics and Astronomy, Dartmouth College, Hanover, NH 03755, USA

5. Space Telescope Science Institute, Baltimore, MD 21218, USA

6. Korea Astronomy and Space Science Institute (KASI), Daejeon 305-348, Korea

7. Center for Astrophysical Sciences, Johns Hopkins University, Baltimore, MD 21218, USA

8. Departamento de Astronomia, Universidad de Concepcion, Casilla 160-C, Concepcion, Chile

9. Department of Physics and Astronomy, Swarthmore College, Swarthmore, PA 19081, USA

Funder

Australian Research Council

CATA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/471/3/3347/19518278/stx1702.pdf

Reference54 articles.

1. An Empirical Pixel-Based Correction for Imperfect CTE. I.HST’s Advanced Camera for Surveys1

2. Centauri: The Population Puzzle Goes Deeper

3. Are the Magellanic Clouds on Their First Passage about the Milky Way?

4. The age of the old Magellanic Cloud clusters -- II. NGC 1786, 1841 and 2210 as evidence for an old coeval population of LMC and galactic globular clusters

5. The relationship between infrared, optical, and ultraviolet extinction

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