Astrophysics and Space Science

, Volume 40, Issue 1, pp 141–148 | Cite as

A new calibration of Wesselink's correlation for the determination of stellar radii

  • Mario Marcocci
  • Italo Mazzitelli


By means of a new homogeneous set of data from 34 double-lined detached systems, we have recalibrated the colour-surface brightness correlation in the interval −0.3≤(B-V)o≤0.95. A comparison is made with Wesselink's calibration. We find that Wesselink's method can provide a good estimate of the stellar radii.


Stellar Radius 
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  1. Giannone, P. and Giannuzzi, M. A.: 1974,Astrophys. Space Sci. 26, 289.Google Scholar
  2. Hanbury Brown, R., Davis, J., Allen, R. S., and Rome, J. M.: 1967,Monthly Notices Roy. Astron. Soc. 137, 408.Google Scholar
  3. Harwood, J. M., Nather, R. E., Walker, A. R., Warner, B., and Wild, P. A. T.: 1975,Monthly Notices Roy. Astron. Soc. 170, 229.Google Scholar
  4. Koch, R. H., Plavec, M., and Wood, F. B.: 1970,A Catalogue of Graded Photometric Studies of Close Binaries, University of Pennsylvania Publications.Google Scholar
  5. Pease, F. G.: 1931,Naturwiss. Berlin 10, 84.Google Scholar
  6. Wesselink, A. J.: 1969,Monthly Notices Roy. Astron. Soc. 144, 297.Google Scholar

Copyright information

© D. Reidel Publishing Company 1976

Authors and Affiliations

  • Mario Marcocci
    • 1
  • Italo Mazzitelli
    • 1
  1. 1.Laboratorio di Astrofisica Spaziale del CNRRomeItaly

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