Journal
ASTROPHYSICAL JOURNAL
Volume 748, Issue 1, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/748/1/69
Keywords
distance scale; globular clusters: individual (NGC 1866); Magellanic Clouds; stars: variables: Cepheids
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Funding
- PRIN-INAF
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We used optical, near-infrared photometry, and radial velocity data for a sample of 11 Cepheids belonging to the young LMC blue populous cluster NGC 1866 to estimate their radii and distances on the basis of the CORS Baade-Wesselink method. This technique, based on an accurate calibration of surface brightness as a function of (U - B), (V - K) colors, allows us to estimate, simultaneously, the linear radius and the angular diameter of Cepheid variables, and consequently to derive their distance. A rigorous error estimate on radii and distances was derived by using Monte Carlo simulations. Our analysis gives a distance modulus for NGC 1866 of 18.51 +/- 0.03 mag, which is in agreement with several independent results.
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