Hostname: page-component-77c89778f8-cnmwb Total loading time: 0 Render date: 2024-07-17T15:00:32.054Z Has data issue: false hasContentIssue false
  • English
  • Français

Attempt to Apply the U B V B1B2V1G Photometry to the Determination of the Distance of the Hyades

Published online by Cambridge University Press:  07 February 2017

M. Golay
M. Golay*
Affiliation:
Observatoire de Genève, Switzerland

Abstract

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.

A photometric method, using the U B V B1B2V1G system, is suggested to determine the distance of clusters. This method based on the assumption that stars with same seven colours have also same absolute visual magnitude is applied, as an example, to Hyades and Praesepe.

Type
Part II: Absolute Magnitudes from Galactic Clusters and Associations
Information
Symposium - International Astronomical Union , Volume 54: Problems of Calibration of Absolute Magnitudes and Temperature of Stars , 1973 , pp. 27 - 30
Copyright
Copyright © Reidel 1973 

References

Bueren, H. G. van: 1952, Bull. Astron. Inst. Neth. 11, 452.Google Scholar
Cowley, A., Cowley, Ch., Jaschek, M., and Jaschek, C.: 1969, Astron. J. 74, 375.Google Scholar
Gliese, W.: 1969, Veröffentl. Astron. Rechen-Inst. Heidelberg , No. 22.Google Scholar
Golay, M.: 1973, this volume, p. 275.CrossRefGoogle Scholar
Golay, M., Peytremann, C., and Maeder, A.: 1969, Publ. Obs. Genève 76.Google Scholar
Hodge, P. W. and Wallerstein, G.: 1966, Publ. Astron. Soc. Pacific 78, 411.CrossRefGoogle Scholar
Klein-Wassink, W. J.: 1927, Publ. Kapteyn Astron. Lab. , No. 4.Google Scholar
Lutz, T. E.: 1970, Astron. J. 75, 1007.Google Scholar
Olsen, E. H.: 1969, , .Google Scholar
Peat, D. W. and Pemberton, A. C.: 1969, Monthly Notices Roy. Astron. Soc. 140, 21.Google Scholar
Rufener, F. G. and Maeder, A.: 1972, in preparation. Google Scholar