Reddening effects in Stromgren photometry

Details Reddening effects in Stromgren photometry Reddening effects in Stromgren photometry

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...241...69a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 241, no. 1, Jan. 1991, p. 69-76. Research supported by DGICYT and Consejeria d

Astronomy and Astrophysics

Astrophysics

7

Astronomical Photometry, B Stars, Interstellar Extinction, Open Clusters, Ubv Spectra, Luminosity, Stellar Envelopes, Stellar Evolution

Scientific paper

The possible existence of systematic errors due to reddening in Stromgren uvby photometric data on B stars is investigated by means of statistical analysis of published observational data on a sample of stars in 17 young open clusters. The data are compiled in tables and graphs and characterized in detail. A linear dependence of the observed reddening slope E(c1)MK/E(b-y)MK on spectral type is found and tentatively attributed to a reddening dependence in the coefficients used to transform instrumental values to standard values.

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