AGB stars in the Magellanic Clouds

Abstract

Some recent results on AGB research in the Magellanic Clouds are reviewed. Discussed are optical and IRAS based surveys, and recent results from the near-infrared DENIS survey, and ISO observations.

Invited Review at the ``ISO's view on Stellar Evolution'' conference, July 1997, Noordwijkerhout, The Netherlands

References in corpus (1)

• Globular Clusters in the Magellanic Clouds.II: IR-Array Photometry for 12 Globulars and Contributions to the Integrated Cluster Light

Cited by in corpus (3)

• Evolution of asymptotic giant branch stars I. Updated synthetic TP-AGB models and their basic calibration
• Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC) II. Cool Evolved Stars
• Effects of thermohaline instability and rotation-induced mixing on the evolution of light elements in the Galaxy : D, 3He and 4He