Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-25T04:58:22.806Z Has data issue: false hasContentIssue false
  • English
  • Français

Stellar distances by the Baade-Wesselink method

Published online by Cambridge University Press:  25 May 2016

G. P. Di Benedetto
G. P. Di Benedetto*
Affiliation:
Istituto di Fisica Cosmica del CNR, Milano, Italy

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.

Galactic and extragalactic distances to Cepheid variable stars according to a modern realization of the geometric Baade-Wesselink method are presented. Reliable results as accurate as few percent are currently achievable, allowing the cosmic distance scale calibration to be significantly improved with respect to previous calibrations.

Type
Stellar Distances
Information
Symposium - International Astronomical Union , Volume 189: Fundamental Stellar Properties: The Interaction Between Observation and Theory , 1997 , pp. 25 - 28
Copyright
Copyright © Kluwer 1997 

References

Davis, J., Tango, W. J.: 1986, Nature 323, 234 Google Scholar
Di Benedetto, G. P., Rabbia, Y.: 1987, Astron. Astrophys. 188, 114 Google Scholar
Di Benedetto, G. P.: 1993, Astron. Astrophys. 270, 315 Google Scholar
Di Benedetto, G. P.: 1994, Astron. Astrophys. 285, 819 Google Scholar
Di Benedetto, G. P.: 1995, Ap. J. 452, 195 CrossRefGoogle Scholar
Gautschy, A.: 1987, Vistas in Astron. 30, 197 Google Scholar
Laney, C. D., Stobie, R. S.: 1995, Mon. Not. R. Astr. Soc. 274, 337 CrossRefGoogle Scholar
Mozurkewich, et. al.: 1991, Astron. J. 101, 2207 Google Scholar
Panagia, et al.: 1996, in The Extragalactic Distance Scale , STScI, May Symp., Baltimore (in press) Google Scholar
Welch, D. L.: 1994, Astron. J. 108, 1421 Google Scholar