Uvby-Beta Photometry of E-Region Stars

Details Uvby-Beta Photometry of E-Region Stars Uvby-Beta Photometry of E-Region Stars

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as..102..637j&link_type=abstract

Astronomy and Astrophysics Supplement, Vol.102, NO.3/DECII, P. 637, 1993

Astronomy and Astrophysics

Astrophysics

13

Photometry

Scientific paper

Photoelectric uvbyβ photometry of 64 E-region stars with V from 6m.2 to 11m.0 covering spectral types from B to M is presented. Comparison with other published results shows that the uvby data presented are closely transformed to the standard system. For the β photometry an offset of 0m.006 may be present. The main purpose of the photoelectric observations is to calibrate the CCD-uvbyβ photometry obtained simultaneously, but the stars may be used as a supplement to the small sample of secondary standard stars for uvbyβ photometry.

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