Hostname: page-component-77c89778f8-n9wrp Total loading time: 0 Render date: 2024-07-16T09:42:03.307Z Has data issue: false hasContentIssue false

Metallicity Effect on Absolute Magnitude Determination

Published online by Cambridge University Press:  04 August 2017

P. Dubois*
Affiliation:
Observatoire de Strasbourg

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Copyright
Copyright © Reidel 1986 

References

Azzopardi, M. and Vigneau, J.: 1975, Astron. Astrohpys. Suppl. Ser. 22, 285 Google Scholar
Balona, I. and Crampton, D.: 1974, Mon. Not. Roy. Astron. Soc. 166, 203 Google Scholar
Buscombe, W. and Kennedy, P.M.: 1962, J. Roy. Astron. Soc. Canada 56, 113 Google Scholar
van den Bergh, B.: 1976, IAU Coll. no.37, p. 13 Google Scholar
Crawford, D.L.: 1973, IAU Symp. no. 54, p. 93 Google Scholar
Crawford, D.L.: 1978, Astron. J. 83, 48 Google Scholar
Dubois, P., Jaschek, M. and Jaschek, C.: 1977, Astron. Astrophys. 60, 205 Google Scholar
Dubois, P.: 1982, Astron. Astrophys. Suppl. Ser. 48, 375 Google Scholar
Fehrenbach, Ch. and Duflot, M.: 1972, Astron. Astrophys. 21, 231 Google Scholar
Humphreys, R.M.: 1983, Astrophys. J. 265, 176 Google Scholar
Hutchings, J.B.: 1966, Mon. Not. Roy. Astron. Soc. 132, 433 Google Scholar
Petrie, R.M.: 1965, Publ. Dom. Astrophys. Obs. 12, 317 Google Scholar
Tully, R.B. and Wolff, S.C.: 1984, Astrophys. J. 281, 67 Google Scholar
Westerlund, B.E., Danziger, I.J. and Graham, J.: 1963, Observatory 83, 74 Google Scholar