This volume reviews the current status with respect to both
theory and observation of the extragalactic distance scale. A
sufficient accuracy is required both for a precise determination of
the cosmological parameters and also in order to achieve a better
understanding of physical processes in extragalactic systems. The
"standard candles," used to set up the extragalactic distance
scale, reviewed in this book include cepheid variables, RR Lyrae
variables, novae, Type Ia and Type II supernovae as well as
globular clusters and planetary nebulae.
General
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