Superbubble dynamics in globular cluster infancy - II. Consequences for secondary star formation in the context of self-enrichment via fast-rotating massive stars
A&A, 552 (2013) A121
Published online: 2013-04-12
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https://doi.org/10.3847/0004-637X/823/1/61
Shape and evolution of wind-blown bubbles of massive stars: on the effect of the interstellar magnetic field
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Galaxies as seen through the most energetic explosions in the universe
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Multiple populations in globular clusters: the distinct kinematic imprints of different formation scenarios
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Globular clusters as the relics of regular star formation in ‘normal’ high-redshift galaxies
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193 (2015)
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Constraining globular cluster formation through studies of young massive clusters – V. ALMA observations of clusters in the Antennae
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Cold gas in hot star clusters: the wind from the red supergiant W26 in Westerlund 1
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A general abundance problem for all self-enrichment scenarios for the origin of multiple populations in globular clusters
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Studying the YMC population of M83: how long clusters remain embedded, their interaction with the ISM and implications for GC formation theories
K. Hollyhead, N. Bastian, A. Adamo, E. Silva-Villa, J. Dale, J. E. Ryon and Z. GazakMonthly Notices of the Royal Astronomical Society 449 (1) 1106 (2015)
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TheHubble Space TelescopeUV Legacy Survey of Galactic Globular Clusters – V. Constraints on formation scenarios
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Evolution of long-lived globular cluster stars
W. Chantereau, C. Charbonnel and T. DecressinAstronomy & Astrophysics 578 A117 (2015)
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The morphology of the sub-giant branch and red clump reveal no sign of age spreads in intermediate-age clusters
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