UVBY beta photometry of southern clusters. VIII - Further data for NGC 3766

Details UVBY beta photometry of southern clusters. VIII - Further data for NGC 3766 UVBY beta photometry of southern clusters. VIII - Further data for NGC 3766

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.225..999s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 225, April 15, 1987, p. 999-1004. Research supported by

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19

B Stars, Star Clusters, Stellar Evolution, Stellar Spectrophotometry

Scientific paper

New uvbyβ data has been collected for 16 stars in NGC 3766 to add to that recently published for 39 other members. They specifically include some of the emission B (Be) stars which were observed for variability by Balona & Englebrecht. The ZAMS is now more clearly defined, as also is the uncommon evolutionary sequence rising vertically at c0 ≡ +0.2.

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