Walraven photometry of OB stars (van Houten, 2001)

Details Walraven photometry of OB stars (van Houten, 2001) Walraven photometry of OB stars (van Houten, 2001)

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ycat..33690527v&link_type=abstract

VizieR On-line Data Catalog: J/A+A/369/527. Originally published in: 2001A&A...369..527V

Physics

Stars: Ob, Photometry: Vbluw

Scientific paper

About 700 stars, mostly OB-stars, were observed by the author at the former Leiden Southern Station at Hartebees poortdam, South Africa, in the observing seasons 1965, 1968, 1969, 1974, 1977, 1978. Observations were made in the five channels of the Walraven photometric system. Due to weathering of the telescope mirror the W channel gave no reliable results for the faintest stars (m=11mag); in these cases the U-W colour index is not given. The change in sensitivity in the V channel, supposedly having occurred in 1968, was not recognised. For a description of the Walraven VBLUW photometric system, see e.g. (1 data file).

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