UBV and H-beta in Sco-Cen association (Slawson+, 1992)

Details UBV and H-beta in Sco-Cen association (Slawson+, 1992) UBV and H-beta in Sco-Cen association (Slawson+, 1992)

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ycat..20820117s&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/82/117. Originally published in: 1992ApJS...82..117S

Physics

Stars: Early-Type, Photometry: Ubv, Photometry: H-Beta

Scientific paper

As part of a thorough study of the luminosity function of Sco-Cen, UBV, and Hβ photometry has been acquired for a large number of mid B- to late A-type stars which are within or surrounding the Scorpius-Centaurus OB association. UBV and Hβ photoelectric measures have been obtained for all the B stars without previous observations and for many of those with in the large field 280deg<=l<=362deg, +10deg<=b<=+40deg, and m-M<=7.5mag. Within the upper Scopius subgroup (ScoOB2), 341deg<=l<=362deg, +10=

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