Electronographic observations of a field in the Small Magellanic Cloud

Details Electronographic observations of a field in the Small Magellanic Cloud Electronographic observations of a field in the Small Magellanic Cloud

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.198..935h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 198, Mar. 1982, p. 935-940.

Astronomy and Astrophysics

Astronomy

18

Electronography, Magellanic Clouds, Star Clusters, Stellar Evolution, Color-Magnitude Diagram, Hertzsprung-Russell Diagram, Star Distribution, Stellar Magnitude, Stellar Spectrophotometry

Scientific paper

A color-magnitude diagram to V approximately 21.5 mag from
electronographs of a field in the western periphery of the Small
Magellanic Cloud shows the presence of a distinct stellar population of
age 3 + or - 1 x 10 to the 9th yr. Some older stars may also be present.
The population appears to be widespread throughout the SMC.

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