The stellar composition in regions of O-associations Cygnus OB4, Cepheus-Lacerta OB1 and Cassiopeia OB9

Details The stellar composition in regions of O-associations Cygnus OB4, Cepheus-Lacerta OB1 and Cassiopeia OB9 The stellar composition in regions of O-associations Cygnus OB4, Cepheus-Lacerta OB1 and Cassiopeia OB9

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8128019r&link_type=abstract

Conf. held in Budapest, 1977 Transl. into ENGLISH from Star Cluster Symp. (Budapest), 1977 p 29-37

Other

Cassiopeia Constellation, Cepheus Constellation, Cygnus Constellation, Hot Stars, Star Clusters, Star Distribution, Stellar Evolution, Stellar Luminosity, Stellar Spectra

Scientific paper

A stellar distribution was made according to spectral and luminosity classes. Three areas of sky were explored. Proceeding from the assumption that a correlation exists between the age of a given star group and the number of hot stars and emission objects in it, it is concluded that the stellar population in the second sky area is of more recent origin than the third. The stellar population in the first area was evidently formed at an earlier time than the others.

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