We present the results of an extensive grid of evolutionary synthesis
models for populations of massive stars. The parameter space has been
chosen to correspond to conditions typically found in objects like gia
nt H II regions, H II galaxies, blue compact dwarf galaxies, nuclear s
tarbursts, and infrared luminous starburst galaxies. The models are ba
sed on the most up-to-date input physics for the theory of stellar atm
ospheres, stellar winds, and stellar evolution. Observable properties
of a population of stars are computed for the two limiting cases of an
instantaneous burst and a constant star-formation rate over a time in
terval of 3 x 10(8) yr. We also investigate the effects of star-format
ion histories which are intermediate between those two extreme cases.
Three choices of the initial mass functions are studied: a Salpeter an
d a Miller-Scalo type IMF with upper mass limits of 100 M(circle dot),
and a Salpeter IMF truncated at 30 M(circle dot). Metallicities of 0.
1 Z(circle dot), 0.25 Z(circle dot) , Z(circle dot), and 2 Z(circle do
t) are considered. The model predictions include the numbers of hot st
ars, supernova rates, colors in the UBVRIJHKL passbands, slopes of the
ultraviolet continuum observable by IUE, HST, and HUT, equivalent wid
ths of hydrogen recombination lines, ionizing fluxes shortward of the
H-0, He-0, and He+ ionization edges, the Lyman discontinuity, and mass
- and energy-deposition rates due to stellar winds and supernovae. We
discuss the contamination of the stellar ultraviolet, optical, and nea
r-infrared continuum by nebular emission. It is found that under typic
al starburst conditions the nebular continuum is not negligible. Depen
ding on the wavelength, addition of the nebular continuum leads to sig
nificantly redder or bluer broadband colors than obtained from a pure
stellar continuum. A population of massive stars is not only important
in terms of its output of radiation but also via its deposition of me
chanical energy. The output of radiative and mechanical luminosity is
compared at various starburst epochs. In a supernova dominated instant
aneous starburst, the mechanical luminosity can be as large as almost
10% of the total radiative luminosity. This occurs when most massive O
stars have disappeared, and the synthetic spectrum in the optical and
near-ultraviolet is dominated by B and A stars. During this epoch, th
e output of ionizing radiation below 912 Angstrom becomes very small,
as indicated by a very large Lyman discontinuity and a very small rati
o of ionizing over mechanical luminosity. We discuss the relevance of
these results for the interpretation of starburst galaxies, active gal
actic nuclei, and the energetics of the interstellar medium.