The nature of star complexes

Details The nature of star complexes The nature of star complexes

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5...21e&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Jan. 1979, p. 21-27.) Soviet Astronomy Letters, vol. 5, Jan.-Feb. 1979, p. 12-16. Tr

Astronomy and Astrophysics

Astronomy

13

Globular Clusters, Star Clusters, Stellar Evolution, Cepheid Variables, Cosmic Gases, Magellanic Clouds, Radial Velocity, Spiral Galaxies, Stellar Luminosity, Stellar Mass

Scientific paper

Several typical star complexes are described and their chief parameters
are estimated. The mass and velocity dispersion have values comparable
with those observed in giant gas complexes, which occur just as often as
star complexes in spiral and irregular galaxies. One can infer that the
star-formation process is concentrated in giant gas complexes.

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