Distances, Ages, and Epoch of Formation of Globular Clusters-Reference-Cited by-同舟云学术

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Distances, Ages, and Epoch of Formation of Globular Clusters

Published:2000-04-10 Issue:1 Volume:533 Page:215-235
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Carretta Eugenio,Gratton Raffaele G.,Clementini Gisella,Fusi Pecci Flavio

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/533/i=1/a=215/pdf

Reference157 articles.

1. The MACHO Project LMC Variable Star Inventory.II.LMC RR Lyrae Stars- Pulsational Characteristics and Indications of a Global Youth of the LMC

2. The MACHO Project Large Magellanic Cloud Variable Star Inventory. III. Multimode RR Lyrae Stars, Distance to the Large Magellanic Cloud, and Age of the Oldest Stars

3. Über eine Möglichkeit, die Pulsationstheorie der δ Cephei-Veränderlichen zu prüfen

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1. JWST Imaging of the Closest Globular Clusters. II. Discovery of Brown Dwarfs in NGC 6397 and Measurement of Age from the Brown Dwarf Cooling Sequence, Using SANDee—A New Grid of Model Isochrones across the Hydrogen-burning Limit;The Astrophysical Journal;2024-08-01

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3. Discovery and Characterization of Two Ultrafaint Dwarfs outside the Halo of the Milky Way: Leo M and Leo K;The Astrophysical Journal;2024-05-30

4. An Empirical Calibration of the Tip of the Red Giant Branch Distance Method in the Near Infrared. I. Hubble Space Telescope WFC3/IR F110W and F160W Filters;The Astrophysical Journal;2024-05-01

5. Symmetry-based study and dynamics of casual bulk viscous matter-dominated universe;The European Physical Journal C;2024-03-30

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