Calibrating the Cepheid period-luminosity relation from the infrared surface brightness technique - II. The effect of metallicity and the distance to the LMC,
A&A, 534 (2011) A95
Published online: 2011-10-11
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The near-infrared detection of PSR B0540–69 and its nebula
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Classical Cepheids, what else?
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QUANTITATIVE SPECTROSCOPY OF BLUE SUPERGIANT STARS IN THE DISK OF M81: METALLICITY, METALLICITY GRADIENT, AND DISTANCE
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Calibrating the Cepheid Period-Luminosity relation from the near-infrared surface brightness technique
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THE CARNEGIE HUBBLE PROGRAM: THE LEAVITT LAW AT 3.6 AND 4.5 μm IN THE MILKY WAY
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The Classical Cepheid Distance scale in the NIR bands
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A GLOBAL PHYSICAL MODEL FOR CEPHEIDS
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RR Lyrae variables in the Small Magellanic Cloud - II. The extended area: chemical and structural analysis
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A discussion on metallicity effects on the period-luminosity relations of Cepheids and Miras
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Cepheid limb darkening, angular diameter corrections, and projection factor from static spherical model stellar atmospheres
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CORS BAADE–WESSELINK DISTANCE TO THE LMC NGC 1866 BLUE POPULOUS CLUSTER
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ON THE APPLICATION OF WESENHEIT FUNCTION IN DERIVING DISTANCE TO GALACTIC CEPHEIDS
Chow-Choong NgeowThe Astrophysical Journal 747 (1) 50 (2012)
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The VMC survey - V. First results for classical Cepheids
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ON THE EVOLUTIONARY AND PULSATION MASS OF CLASSICAL CEPHEIDS. III. THE CASE OF THE ECLIPSING BINARY CEPHEID CEP0227 IN THE LARGE MAGELLANIC CLOUD
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Cepheid distances from the Baade–Wesselink method
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THE ARAUCARIA PROJECT: AN ACCURATE DISTANCE TO THE LATE-TYPE DOUBLE-LINED ECLIPSING BINARY OGLE SMC113.3 4007 IN THE SMALL MAGELLANIC CLOUD
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