Stromgren Photometry of Cool White Dwarfs

Details Stromgren Photometry of Cool White Dwarfs Stromgren Photometry of Cool White Dwarfs

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26as...43..367l&link_type=abstract

Astronomy and Astrophysics Supplement, Vol. 43, P. 367, 1981

Astronomy and Astrophysics

Astrophysics

25

Scientific paper

Strömgren photometric data are given for a selected group of 30 white dwarfs. This sample consists mostly of nearby, cool, non-DA stars. In addition, colors for 16 more white dwarfs are compared to those obtained by other authors. By comparing the response of our local photometric system to that of the standard Strömgren system, it is found that different transformation coefficients must be used for DA and non-DA stars. It is suggested that greater accuracy could be obtained if the spectral types of the stars are taken into account in future observations of white dwarfs.

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