Kinematic Analysis of Cepheus OB3

Details Kinematic Analysis of Cepheus OB3 Kinematic Analysis of Cepheus OB3

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997esasp.402..299t&link_type=abstract

Proceedings of the ESA Symposium `Hipparcos - Venice '97', 13-16 May, Venice, Italy, ESA SP-402 (July 1997), p. 299-302

Computer Science

1

Scientific paper

24 early type stars were selected in the Cepheus OB3 region and the surrounding area on the basis of their relationship to the Cepheus OB3 association or their photometric compatiblility with this group. A kinematic study using Hipparcos data did not show significant differences between the well known members and the remaining stars. Because some stars overlap Cepheus OB2 region, a connexion between both groups cannot be ruled out. Kinematic ages for the young and old subgroups are computed.

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