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New grids of stellar models. II.
New stellar models spefically designed for the Small Magellanic Cloud are presented in this paper. In order to take into account the uncertainties in the metal content we... -
Stellar models grids. Z=0.02, M=0.8 to 125
We present new stellar models based on updated physics (opacities, expanded nuclear network and mass loss rates). We compute stellar models suitable for the mean solar... -
BVIJHK properties of Single Stellar Populations
We describe a large grid of photometric properties of single stellar populations that focuses on the near infrared properties of intermediate age populations. The underlying... -
Radial oscillations of relativistic stars
We present a new survey of the radial oscillation modes of neutron stars. This study complements and corrects earlier studies of radial oscillations. We present an extensive... -
Dust formation in WC stars
The following table gives the ratefile of the chemical model. Columns {alpha}, {beta} and {gamma} give the rate k at temperature T in the Arrhenius form: k = {alpha} *... -
PSR J1012+5307 evolutionary tracks
We present a set of evolutionary tracks for white dwarfs with helium cores in the mass range from 0.179 to 0.414M_{sun}. The tracks are based on a 1M{sun}_ model sequence... -
Low-mass stars evolutionary models
Physical properties and absolute magnitudes of low-mass stars for different initial metallicity [M/H], helium mass fraction Y and mixing length parameter Lmix: mass (in solar... -
Star cluster evolution
A model of spectral evolution of star forming galaxies of various metallicity has been used to study the relation between the optical emission line ratio... -
Evolution models of elliptical galaxies. II.
In this paper we present new chemo-spectro-photometric models of elliptical galaxies in which infall of primordial gas is allowed to occur. They aim to simulate the collapse of... -
Stellar evolution. II. Post-AGB
We present a set of evolutionary tracks for central stars of planetary nebulae in the range from 0.53 to 0.94M_{sun}. These models are based on extensive stellar evolution... -
Rotating neutron stars models. I.
(no description available) -
Isochrone database for single- and binary-star SSPs
We first presented an isochrone data base that can be widely used for stellar population synthesis studies and colour-magnitude diagram (CMD) fitting. The data base consists of... -
Star formation in galaxies
Evolutionary models of disk galaxies are presented (table3), and are confronted with a sample of late type galaxies from the Tully (Nearby Galaxies, see Cat. ) and the de... -
Low-mass stars
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Library of Lick/IDS indices for binaries
Using evolutionary population synthesis, we present 13 refined absorption-line indices defined by the Lick Observatory Image Dissector Scanner (Lick/IDS) system for an extensive... -
Stellar evolution models for Z = 0.0001 to 0.03
We have calculated a grid of empirically well tested evolutionary tracks with masses M between 0.5 and 50M_{sun}_, spaced by approximately 0.1 in log M, and with metallicities... -
Population model of binary stars in the Galaxy
A comparative study of the population of the galactic binary stars is performed for two modes of star formation: star formation at a constant rate over 10^+10^yrs, and a burst... -
Post-AGB evolution
In this paper, we present the results for the post-AGB phases of stellar evolutionary sequences, complete from the main-sequence phase, through the AGB phase, and on into the... -
Variations on debris disks. II.
We describe comprehensive calculations of the formation of icy planets and debris disks at 30-150AU around 1-3M_{sun}_ stars. Disks composed of large, strong planetesimals... -
Predicted IR excesses for protoplanetary disks
We describe calculations for the formation of icy planets and debris disks at 30-150AU around 1-3M_{sun} stars. Debris disk formation coincides with the formation of planetary...
