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Metallicity Effect on Absolute Magnitude Determination
Published online by Cambridge University Press: 04 August 2017
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In our Galaxy, it is possible to determine the absolute magnitude of a star by mean of the intensity of the hydrogen lines, if we know the spectral type of the star or its temperature (see for instance Petrie, 1965; Hutchings, 1966; Balona and Crampton, 1974; Crawford, 1973, 1978; …).
- Type
- Poster Papers 3
- Information
- Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 415 - 416
- Copyright
- Copyright © Reidel 1986