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- W1627808250 abstract "Observations of 22 DB stars using the uvby photometric system are discussed. In the [( b – y ),( u – b )] diagram, these objects define a relatively tight sequence, but the interpretation is hampered by the lack of a precise knowledge of atmospheric element abundances in these stars. The recent models of Koester (1979) show a larger gravity separation for the DB’s using Strömgren photometry and appear to fit the observations better than earlier theoretical results. Due to the tightness of the DB sequence at the hot and cool ends, respectively, there appears to be evidence for restricted ranges in log g and the atmospheric hydrogen abundance." @default.
- W1627808250 created "2016-06-24" @default.
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- W1627808250 date "1979-08-01" @default.
- W1627808250 modified "2023-09-28" @default.
- W1627808250 title "Four Color Photometry of DB White Dwarfs" @default.
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- W1627808250 doi "https://doi.org/10.1017/s0252921100075990" @default.
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