Absolute Magnitude Calibration from H-Beta Photometry of Open Star Clusters

Details Absolute Magnitude Calibration from H-Beta Photometry of Open Star Clusters Absolute Magnitude Calibration from H-Beta Photometry of Open Star Clusters

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987bicds..33...41m&link_type=abstract

Bulletin d'Information du Centre de Donnees Stellaires, Vol. 33, p.41

Computer Science

1

Scientific paper

The (MV,Hß) calibrations are briefly reviewed and compared. The Hß data available for each cluster have also been intercompared and the results are given in a tabular form. Most zero point differences are smaller than 0.010 and the dispersion over the mean is comprised between 0.005 and 0.015. This means that erratic errors of several hundredths of magnitude do exist, resulting in large errors on absolute magnitude determination.

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