An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars
A&A, 438 1 (2005) 273-289
Published online: 2005-07-06
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THE RED SUPERGIANT CONTENT OF M31*
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Multiple Stellar Populations and Their Evolution in Globular Clusters: A Nucleosynthesis Perspective
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GALEXDETECTION OF SHOCK BREAKOUT IN TYPE IIP SUPERNOVA PS1-13arp: IMPLICATIONS FOR THE PROGENITOR STAR WIND
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CAN STAR CLUSTER ENVIRONMENT AFFECT DUST INPUT FROM MASSIVE AGB STARS?
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THE DUSTIEST POST-MAIN SEQUENCE STARS IN THE MAGELLANIC CLOUDS
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