Developments in the research of star clusters between 1964 and 1979

Details Developments in the research of star clusters between 1964 and 1979 Developments in the research of star clusters between 1964 and 1979

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980s%26w....19..162s&link_type=abstract

Sterne und Weltraum, vol. 19, May 1980, p.162-167. In German.

Other

Globular Clusters, Main Sequence Stars, Star Clusters, Stellar Evolution, Astronomical Catalogs, Binary Stars, Milky Way Galaxy, Open Clusters, Star Distribution, Uhuru Satellite, X Ray Stars

Scientific paper

Several features in globular and open star cluster research are examined. The development of the main sequence is discussed in three stages, hydrogen burning in the center of the star, contraction of short duration, and hydrogen burning from a thick shell source. Data from seven X-ray emission sources are presented whose positions coincide with globular clusters. X-ray emission research with the UHURU satellite is also considered. The frequency gradient of elements in the Milky Way is investigated with emphasis on the decrease of frequency towards the outer boundaries. The globular cluster catalog of Harris and Racine (1979) is recommended along with others.

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