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A compilation of charged-particle induced thermonuclear reaction rates
Low-energy cross section data for 86 charged-particle induced reactions involving light (1 less than or equal to Z less than or equal to 14), mostly stable, nuclei are compiled. The correspondingExpand
The Pisa pre-main sequence tracks and isochrones - A database covering a wide range of Z, Y, mass, and age values
Context. In recent years new observations of pre-main sequence stars (pre-MS) with Z≤ Z⊙ have been made available. To take full advantage of the continuously growing amount of data of pre-MS stars inExpand
GALACTIC GLOBULAR CLUSTER STARS : FROM THEORY TO OBSERVATION
We use evolutionary calculations presented in a recent paper (Cassisi et al. 1997a: hereinafter Paper I) to predict B, V , I magnitudes for stars in galactic glob- ulars. The eect of the adoptedExpand
A pulsational approach to near-infrared and visual magnitudes of RR Lyr stars
In this paper, we present an improved theoretical scenario concerning near-infrared and visual magnitudes of RR Lyr variables, as based on up-to-date pulsating models. New relations connecting V andExpand
An updated theoretical scenario for globular cluster stars
In the rst part of this paper we revisit the history of theoretical predictions for HB luminosities in old Population II stellar clusters, starting from the results of \old" evolutionary computationsExpand
ON THE DISTANCE AND REDDENING OF THE STARBURST GALAXY IC 10
We present deep and accurate optical photometry of the Local Group starburst galaxy IC 10. The photometry is based on two sets of images collected with the Advanced Camera for Surveys and with theExpand
STRÖMGREN PHOTOMETRY OF GALACTIC GLOBULAR CLUSTERS. II. METALLICITY DISTRIBUTION OF RED GIANTS IN ω CENTAURI
We present new intermediate-band Str?mgren photometry based on more than 300 u, v, b, y images of the Galactic globular cluster ? Cen. Optical data were supplemented with new multiband near-infraredExpand
PHOTOMETRIC DETERMINATION OF THE MASS ACCRETION RATES OF PRE-MAIN-SEQUENCE STARS. II. NGC 346 IN THE SMALL MAGELLANIC CLOUD*
We have studied the properties of the stellar populations in the field of the NGC 346 cluster in the Small Magellanic Cloud, using a novel self-consistent method that allows us to reliably identifyExpand
Hipparcos open clusters and stellar evolution
By relying on recently improved Hipparcos parallaxes for the Hyades, Pleiades and Ursa Major clusters we find that stellar models with updated physical inputs nicely reproduce the location in theExpand
Statistical errors and systematic biases in the calibration of the convective core overshooting with eclipsing binaries - A case study: TZ Fornacis
We attempt to constrain the initial helium abundance, the age and the efficiency of the convective core overshooting of the binary system TZ Fornacis. Our main aim is in pointing out the biases inExpand
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