By means of a population synthesis code, we have carried out a theoretical study of semi-detached symbiotic stars, detached symbiotic stars and D-symbiotic stars.
First, we present the integrated color indices, the spectral energy distributions (ISEDs) and 21 Lick/IDS absorption-line indices for an extensive set of instantaneous burst SSPs.
At last, we include binary interactions in our EPS models to investigate the effects on the integrated colours, ISEDs and Lick absorption feature indices.
The results indicate that the continuum flux fraction at 5870 A owing to an old component is ~ 64%, and that of very young components (T<108yr)is<1%, respectively.
It is also pointed out that since a similar equation governs the continuum spectra emitted by a distribution of black-body radiators, the analysis is relevant to the problem of stellar population synthesis from galactic spectra.
We outline the revised physical assumption which have been incorporated into our previously published evolutionary model for stellar population synthesis in galaxies.
We present a stellar population synthesis model for the UV spectrum of the peculiar galaxy NGC 1672, computed with the use of theIUE Atlas Library of Stellar Spectra.
We investigate the consequences of a truncated initial mass function on the photometric evolution of starburst galaxies using new models of stellar population synthesis.
The population synthesis method is used to study the possibility of explaining the appreciable fraction of the intergalactic type-Ia supernovae (SN Ia), 20-15+12%, observed in galaxy clusters (Gal-Yam et al.
Population synthesis is used to model the number of neutron stars in globular clusters that are observed as low-mass X-ray sources and millisecond radio pulsars.
We apply a population synthesis technique to study the formation and evolution of low-mass X-ray binaries with black holes, observed as X-ray novae, from hierarchical triple systems.