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Binary evolution
Using Eggleton's stellar evolution code, we carry out 150 runs of Population I binary evolution calculations with the initial primary mass between 1 and 8 solar masses, the... -
Stellar composition of CMa R1
This directory contains movies in mpeg format which show models for the time evolution of the Hertzsprung-Russell diagram of a very young open cluster between 0 and 30Myr. Four... -
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... -
FRII radio sources dynamical models
Dynamical evolution models of 361 extragalactic Fanaroff-Riley type II radio sources selected from the Cambridge 3CRR, 6CE, 5C6, and 5C7 Sky Surveys, as well as the Bologna B2,... -
Bulge+disk decompositions of SDSS galaxies
We perform two-dimensional, point-spread-function-convolved, bulge+disk decompositions in the g and r bandpasses on a sample of 1123718 galaxies from the Legacy area of 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... -
Population synthesis in the blue. IV
We present a new set of model predictions for 16 Lick absorption line indices from H{delta} through Fe5335 and UBV colors for single stellar populations with ages ranging... -
Emission lines of evolving HII regions
We build, as far as theory will permit, self-consistent model HII regions around central clusters of aging stars. These produce strong emission line diagnostics applicable to... -
Optically thick winds from degenerate dwarfs. I.
Twenty-six sequences of optically thick wind solutions have been calculated which mimic the time-dependent evolution of classical novae of populations I and II. The peak of the... -
Chemo-evolutionary Population Synthesis II.
We present the results of applying a new chemo-evolutionary stellar population model, developed in a previous paper, to new high-quality observational data of the nuclear... -
Cosmic background anisotropies
Cosmic microwave background (CMB) anisotropies and density fluctuations are calculated for flat cold dark matter (CDM) models with a wide range of parameters, viz., {OMEGA}0,h,... -
TESS obs. & rotational periods of T Tauri in Orion
We present a large-scale study of stellar rotation for T Tauri stars in the Orion star-forming complex. We use the projected rotational velocity (vsin(i)) estimations reported... -
Adiabatic Mass Loss in Binary Stars. III.
The distinguishing feature of the evolution of close binary stars is the role played by the mass exchange between the component stars. Whether or not the mass transfer is... -
OGLE LMC-T2CEP-211 eclipsing binary LCs and RVs
We present the analysis of a peculiar W Virginis (pWVir) type II Cepheid, OGLE-LMC-T2CEP-211 (P_puls_=9.393d), in a double-lined binary system (P_orb_=242d), which shed light on... -
X-ray stacking analysis of Chandra-COSMOS gal.
We present an X-ray stacking analysis of ~75000 star-forming galaxies between 0.1<z<5.0 using the Chandra COSMOS-Legacy survey to study the X-ray emission of... -
Stellar yields of rotating first stars. II.
Recent theory predicts that first stars are born with a massive initial mass of >~100M_{sun}. Pair-instability supernova (PISN) is a common fate for such massive stars. Our... -
Tracers of stellar mass-loss. II.
I present integrated colors and surface brightness fluctuation magnitudes in the mid-infrared (IR), derived from stellar population synthesis models that include the effects of... -
Yields of Fe and Zn for different types of SNe
The heaviest iron-peak element Zinc (Zn) has been used as an important tracer of cosmic chemical evolution. Spectroscopic observations of the metal-poor stars in Local Group...
