Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-26T04:02:18.163Z Has data issue: false hasContentIssue false
  • English
  • Français

Absolute Magnitudes of O Stars from a Study of Visual Multiple Systems

Published online by Cambridge University Press:  07 February 2017

M. L. Burnichon
M. L. Burnichon*
Affiliation:
Institut d'Astrophysique de Paris, France

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.

From a careful study of physical multiple systems, it has been possible to derive differentially absolute magnitudes and intrinsic colours of O stars from the corresponding quantities, relatively well-known, of companions of these stars.

Type
Part IV: Absolute Magnitude Determinations from Hydrogen-Line Photometry
Information
Symposium - International Astronomical Union , Volume 54: Problems of Calibration of Absolute Magnitudes and Temperature of Stars , 1973 , pp. 126 - 127
Copyright
Copyright © Reidel 1973 

References

Burnichon, M. L.: 1972, ‘Contribution à l'étude des couleurs intrinsèques et des magnitudes absolues des étoiles bleues de grande luminosité à partir de l'observation de systèmes multiples’, Thèse.Google Scholar
Chalonge, D. and Divan, L.: 1973, Astron. Astrophys. 23, 69.Google Scholar