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Astrophysics and Space Science

, Volume 263, Issue 1–4, pp 259–262 | Cite as

Radial Velocity Measurements with FXCOR

  • José J. Rodes
  • Guillermo Bernabeu
  • Juan Fabregat
Article

Abstract

We present measured radial velocities of two peculiar early B type stars, to check their membership to the open cluster NGC 663. The radial velocities have been obtained with the cross correlation technique, using as a template stars from the list of Liu et al. (1989).

We have obtained accuracies around 3-4 km/s in our radial velocity measurements. From our results we conclude that both stars are probably non members of the cluster.

Keywords

Cross Correlation Radial Velocity Velocity Measurement Open Cluster Correlation Technique 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Corbet, R.H.D., 1986, MNRAS, 220, 1047ADSGoogle Scholar
  2. Fabregat, Juan et al., 1996, A&ASS, 119, 1Google Scholar
  3. Liu, T., Janes, K.A., Bania, T.M., 1989, AJ, 98, 626CrossRefADSGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1998

Authors and Affiliations

  • José J. Rodes
    • 1
  • Guillermo Bernabeu
    • 1
  • Juan Fabregat
    • 2
  1. 1.Departament de Física, Enginyeria de sistemes i Teoria del senyalUniversitat d'AlacantSpain
  2. 2.Departament d'Astronomía i AstrofísicaUniversitat de ValènciaSpain

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