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Cited article:

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 III, M. Gómez

A&A, 440 2 (2005) 487-498

Published online: 2005-09-01

DOI: https://doi.org/10.1051/0004-6361:20053067

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Theoretical fit of Cepheid light and radial velocity curves in the Large Magellanic Cloud cluster NGC 1866

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Binarity among Cepheids in the Magellanic Clouds

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Detailed chemical composition of classical Cepheids in the LMC cluster NGC 1866 and in the field of the SMC

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