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- W133737526 abstract "In the preceeding paper of this Symposium by Cayrel and Perrin (1978), HR diagrams have been discussed, in which the [Fe/H] ratio and effective temperatures are derived from model atmosphere analyses and absolute bolometric magnitude from apparent visual magnitude, parallax and bolometric correction. The use of parallaxes imposes a very severe restriction on the number of objects, as parallaxes of at least 0″.050 are needed to have an absolute magnitude good to ±0 m .4." @default.
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- W133737526 date "1978-01-01" @default.
- W133737526 modified "2023-09-25" @default.
- W133737526 title "Is it Possible to Derive the Position of a Star in the HR Diagram from Multicolor Photometry?" @default.
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- W133737526 doi "https://doi.org/10.1017/s0074180900145723" @default.
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