Kamath, DevikaWood, Peter RSoszyński, IgorLebzelter, Thomas2015-12-100035-8711http://hdl.handle.net/1885/57230The intermediate-age Magellanic Cloud clusters NGC 1978 and 419 are each found to contain substantial numbers of pulsating asymptotic giant branch (AGB) stars, both oxygen rich and carbon rich. Each cluster also contains two pulsating AGB stars which areKeywords: Galaxies: star clusters: individual: NGC 1978; Galaxies: star clusters: individual: NGC 419; Magellanic Clouds; Stars: AGB and post-AGB; Stars: mass-loss; Stars: variables: general201010.1111/j.1365-2966.2010.17137.x2016-02-24