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Cited article:
M. A. T. Groenewegen , M. Salaris
A&A, 410 3 (2003) 887-896
Published online: 2003-11-17
This article has been cited by the following article(s):
14 articles
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ON THE ENHANCEMENT OF MASS LOSS IN CEPHEIDS DUE TO RADIAL PULSATION. II. THE EFFECT OF METALLICITY
Hilding R. Neilson and John B. Lester The Astrophysical Journal 690 (2) 1829 (2009) https://doi.org/10.1088/0004-637X/690/2/1829
A PROBLEM WITH THE CLUSTERING OF RECENT MEASURES OF THE DISTANCE TO THE LARGE MAGELLANIC CLOUD
Bradley E. Schaefer The Astronomical Journal 135 (1) 112 (2008) https://doi.org/10.1088/0004-6256/135/1/112
Comparison of Distances from RR Lyrae Stars, the Tip of the Red Giant Branch, and Classical Cepheids
G. A. Tammann, Allan Sandage and B. Reindl The Astrophysical Journal 679 (1) 52 (2008) https://doi.org/10.1086/529508
The projection factor, period–radius relation, and surface–brightness colour relation in classical cepheids
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The evolution of binary star clusters and the nature of NGC 2136/NGC 2137
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Infrared photometry of Cepheids in the LMC clusters NGC 1866 and NGC 2031
V. Testa, M. Marconi, I. Musella, et al. Astronomy & Astrophysics 462 (2) 599 (2007) https://doi.org/10.1051/0004-6361:20066114
Direct Distances to Cepheids in the Large Magellanic Cloud: Evidence for a Universal Slope of the Period‐Luminosity Relation up to Solar Abundance
Wolfgang Gieren, Jesper Storm, Thomas G. Barnes III, et al. The Astrophysical Journal 627 (1) 224 (2005) https://doi.org/10.1086/430496
The near-IR surface brightness method applied to six Cepheids in the young LMC cluster NGC 1866
J. Storm, W. P. Gieren, P. Fouqué, T. G. Barnes and M. Gómez Astronomy & Astrophysics 440 (2) 487 (2005) https://doi.org/10.1051/0004-6361:20053067
A review of the distance and structure of the Large Magellanic Cloud
David R Alves New Astronomy Reviews 48 (9) 659 (2004) https://doi.org/10.1016/j.newar.2004.03.001
New period-luminosity and period-color relations of classical Cepheids
A. Sandage, G. A. Tammann and B. Reindl Astronomy & Astrophysics 424 (1) 43 (2004) https://doi.org/10.1051/0004-6361:20040222