Infrared photometry of Cepheids in the LMC clusters NGC 1866 and NGC 2031
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20066114/pdf
Reference56 articles.
1. A review of the distance and structure of the Large Magellanic Cloud
2. The Star Cluster NGC 1866 and its Cepheids
3. NGC 1866: A workbench for stellar evolution
4. Theoretical Models for Classical Cepheids. II. Period‐Luminosity, Period‐Color, and Period‐Luminosity‐Color Relations
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1. Metallicity estimations of MW, SMC, and LMC classical Cepheids from the shape of the V- and I-band light curves;Astronomy & Astrophysics;2023-03
2. Kinematic Structure of the Large Magellanic Cloud Globular Cluster System from Gaia eDR3 and Hubble Space Telescope Proper Motions;The Astrophysical Journal;2022-08-01
3. On the dynamical evolution of Cepheids in star clusters;Astronomy & Astrophysics;2022-03
4. On Cepheid Distance Scale Bias Due to Stellar Companions and Cluster Populations;The Astrophysical Journal;2018-06-28
5. The Cepheids of NGC 1866: a precise benchmark for the extragalactic distance scale and stellar evolution from modernUBVIphotometry;Monthly Notices of the Royal Astronomical Society;2016-02-18
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