The distance to the LMC cluster NGC 1866; clues from the cluster Cepheid population
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20031332/pdf
Reference46 articles.
1. [ITAL]K[/ITAL]-Band Red Clump Distance to the Large Magellanic Cloud
2. The Star Cluster NGC 1866 and its Cepheids
3. Astrometry with the [ITAL]Hubble Space Telescope[/ITAL]: A Parallax of the Fundamental Distance Calibrator RR Lyrae
4. Integrated UBV Photometry of 624 Star Clusters and Associations in the Large Magellanic Cloud
5. Binney, J., & Merrifield, M. 1998, in Galactic Astronomy, Princeton Series in Astrophysics (Princeton University Press), 106
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3. Theoretical fit of Cepheid light and radial velocity curves in the Large Magellanic Cloud cluster NGC 1866;Monthly Notices of the Royal Astronomical Society;2012-11-07
4. CORS BAADE–WESSELINK DISTANCE TO THE LMC NGC 1866 BLUE POPULOUS CLUSTER;The Astrophysical Journal;2012-03-06
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