Detection and photometry of red giants in the Magellanic Clouds

Details Detection and photometry of red giants in the Magellanic Clouds Detection and photometry of red giants in the Magellanic Clouds

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..183a&link_type=abstract

IN: Structure and evolution of the Magellanic Clouds; Proceedings of the Symposium, Tuebingen, West Germany, September 5-8, 1983

Astronomy and Astrophysics

Astronomy

7

Astronomical Photometry, Magellanic Clouds, Red Giant Stars, Stellar Evolution, Carbon Stars, Star Clusters, Star Formation Rate, Stellar Color, Stellar Luminosity

Scientific paper

This review will focus on photometric observations of evolved stars in the Magellanic Clouds. Emphasis is placed on red and near-infrared measurements, as these allow reasonable estimates to be made of bolometric magnitude and temperature for reliable placement in the physical HR diagram. The review is divided into three parts: field stars, cluster stars, and red variables; a summary of the surveys for objects in each of these areas is also given. Particular attention is drawn to the intermediate-age stellar population, as this component appears to be the primary tracer of the star formation rate and chemical enrichment history of the Clouds.

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