The pulsation of AGB stars in the Magellanic Cloud clusters NGC 1978 and 419
The 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 are
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Kamath_The_pulsation_of_AGB_stars_in_2010.pdf||1.45 MB||Adobe PDF||Request a copy|
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