A study of the young open cluster NGC 6611

Details A study of the young open cluster NGC 6611 A study of the young open cluster NGC 6611

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..66....3s&link_type=abstract

Astrophysics and Space Science, vol. 66, no. 1, Nov. 1979, p. 3-12.

Mathematics

Probability

40

Open Clusters, Star Distribution, Stellar Luminosity, Stellar Spectrophotometry, Ubv Spectra, Electrophotometry, Main Sequence Stars, Probability Distribution Functions, Stellar Magnitude

Scientific paper

Photoelectric magnitudes and colours in the UBV system have been determined for 50 stars in NGC 6611. The reddening value varies across the cluster from E(B-V) = 0.58m to E(B-V) = 1.21m. The distance modulus to the cluster is estimated at 12.5 + or - 0.2m. It is found that cluster stars are not of the same age. The cluster luminosity function is compared with the general and initial luminosity functions.

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