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- W3098808441 endingPage "A75" @default.
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- W3098808441 abstract "Context. Starbursts play an essential role in the evolution of galaxies. In these environments, massive stars, with their short lifetimes, are of particular importance. The stellar winds of massive stars significantly influence not only on their surroundings, but the associated mass loss also profoundly affects the evolution of the stars themselves. The evolution of the dense cores of massive starburst clusters is also affected by dynamical processes induced by N-body interactions, in addition to the evolution of each star, and the formation of very massive stars with masses up to several thousand solar masses may be decisive for the evolution of the cluster. The interpretation of the corresponding observations relies mainly on the theoretical modeling of such starbursts, which is a major challenge." @default.
- W3098808441 created "2020-11-23" @default.
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- W3098808441 date "2012-02-01" @default.
- W3098808441 modified "2023-10-01" @default.
- W3098808441 title "Radiation-driven winds of hot luminous stars XVI. Expanding atmospheres of massive and very massive stars and the evolution of dense stellar clusters" @default.
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- W3098808441 doi "https://doi.org/10.1051/0004-6361/201117621" @default.
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