Estimated astrophysical parameters from uvby (Philip+ 1980)

Computer Science

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Photometry: Uvby: Beta, Effective Temperatures

Scientific paper

Observed values of the Stroemgren uvby colors were collected from the literature. A computer program calculated the reddening for each star. This value was used to compute the unreddened value of (b-v), c1, and m1. These were then used to compute [c(1)], [m(1)], and [u-b] for the star. Except for the H beta index, the observed quantities are not included.
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