Walraven photometry in Sco-Cen association (De Geus+, 1989)

Details Walraven photometry in Sco-Cen association (De Geus+, 1989) Walraven photometry in Sco-Cen association (De Geus+, 1989)

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..32160044d&link_type=abstract

VizieR On-line Data Catalog: J/A+A/216/44. Originally published in: 1989A&A...216...44D

Physics

Associations: Stellar, Photometry: Vbluw, Effective Temperatures

Scientific paper

Stars in the Sco-Cen association were observed in the Walraven photometric system during several observing sessions during the months of April tp August in the years 1983 to 1987. The five bands V B L U W are observed simultaneously, and the mean rms errors are 0.0016 in V, 0.0008 in (V-B), 0.0010 in (B-U), 0.0009 in (U-W) and 0.0007 in (B-L). The physical parameters Teff, log(g), luminosity, distances and membership are derived.
(3 data files).

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