CCD photometry of the young association NGC 1962-65-66-70 in the Large Magellanic Cloud.

Details CCD photometry of the young association NGC 1962-65-66-70 in the Large Magellanic Cloud. CCD photometry of the young association NGC 1962-65-66-70 in the Large Magellanic Cloud.

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...301..396w&link_type=abstract

Astronomy and Astrophysics, v.301, p.396

Astronomy and Astrophysics

Astrophysics

9

Magellanic Clouds, Galaxies: Star Clusters, Open Clusters And Associations: Individual: Ngc 1962-, 5-66-70, Stars: Luminosity Function, Mass Function, Stars: Individual: Hde 269551

Scientific paper

We present CCD data in the Johnson passbands B and V of the young association NGC 1962-65-66-70 in the Large Magellanic Cloud. We find the association to show an age spread in the range 4 to 9Myr. Some signs for a propagation of star formation from the south-eastern to the northern part of the region can be found, but they are based on very few stars. The slope of the luminosity function is γ=0.27+/-0.02 for stars of the magnitude range -8

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