Electronographic photometry in the galactic cluster M 37

Details Electronographic photometry in the galactic cluster M 37 Electronographic photometry in the galactic cluster M 37

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...50..251r&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 50, Nov. 1982, p. 251-260.

Astronomy and Astrophysics

Astrophysics

3

Astrometry, Astronomical Photometry, Electronography, Galactic Clusters, Stellar Magnitude, Open Clusters, Photographic Plates, Ubv Spectra

Scientific paper

Results are reported for measurements of 92 stars on two sets of U, B, and V electronographic plates of the open cluster M37 that were performed to obtain a photometric sequence in the direction of the galactic anticenter. A sequence of 69 stars in B and V with magnitudes of 13.3 to 20.9 in B and of 12.8 to 19.7 in V is obtained, along with a sequence of 43 of the 69 stars in U with U magnitudes of 13.5 to 18.9. The accuracies are shown to be 0.055 mag in V, 0.075 mag in B, and 0.10 mag in U.

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