Add to ORKGWe continue our series of papers on open cluster distances by comparing multicolor photometry of single stars in the Hyades with theoretical isochrones constructed with various color-temperature relations. After verifying that the isochrone effective temperatures agree well with spectroscopically determined values, we argue that mismatches between the photometry and the theoretical colors likely arise from systematic errors in the color-temperature relations.We then describe a method for empirically correcting the isochrones to match the photometry and discuss the dependence of the isochrone luminosity on metallicity
11 pages, 5 figuresInternational audienceMetallicity is one of four free parameters typically consid...
We present a new technique to fit color–magnitude diagrams of open clusters based on the cross-entr...
Context.With the $\Delta a$ photometric system, it is possible to study very distant galactic and ev...
We continue our series of papers on open cluster distances by comparing multicolor photometry of sin...
We continue our series of papers on open cluster distances with a critical assessment of the accurac...
Current generation stellar isochrone models exhibit non-negligible discrepancies due to variations i...
We continue our series of papers on open cluster distances with a critical assessment of the accurac...
In the first of a new series of papers on open cluster distances, we use updated stellar evolution m...
The increase in high-quality VI-photometry for globular clusters requires the transformation of theo...
We study classical disk clusters at nearly solar metallicity with ages in the range 200 Myr – 6Gyr u...
International audienceWe perform an extensive test of theoretical stellar models for main-sequence (...
In the last decades we witnessed an increase in studies of open clusters of the Galaxy, especially b...
We present new $BV(RI)_{\rm C}$ photometry for a sample of 54 local G and K stars with accurate Hip...
We have combined existing optical magnitudes for stars in seven open clusters and 54 field stars wit...
Abstract. In recent years, several authors have revised the calibrations used to compute physical pa...
11 pages, 5 figuresInternational audienceMetallicity is one of four free parameters typically consid...
We present a new technique to fit color–magnitude diagrams of open clusters based on the cross-entr...
Context.With the $\Delta a$ photometric system, it is possible to study very distant galactic and ev...
We continue our series of papers on open cluster distances by comparing multicolor photometry of sin...
We continue our series of papers on open cluster distances with a critical assessment of the accurac...
Current generation stellar isochrone models exhibit non-negligible discrepancies due to variations i...
We continue our series of papers on open cluster distances with a critical assessment of the accurac...
In the first of a new series of papers on open cluster distances, we use updated stellar evolution m...
The increase in high-quality VI-photometry for globular clusters requires the transformation of theo...
We study classical disk clusters at nearly solar metallicity with ages in the range 200 Myr – 6Gyr u...
International audienceWe perform an extensive test of theoretical stellar models for main-sequence (...
In the last decades we witnessed an increase in studies of open clusters of the Galaxy, especially b...
We present new $BV(RI)_{\rm C}$ photometry for a sample of 54 local G and K stars with accurate Hip...
We have combined existing optical magnitudes for stars in seven open clusters and 54 field stars wit...
Abstract. In recent years, several authors have revised the calibrations used to compute physical pa...
11 pages, 5 figuresInternational audienceMetallicity is one of four free parameters typically consid...
We present a new technique to fit color–magnitude diagrams of open clusters based on the cross-entr...
Context.With the $\Delta a$ photometric system, it is possible to study very distant galactic and ev...