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- W1560761392 abstract "The Magellanic Clouds represent the best laboratories to study the metallicity effect on the late evolution of massive stars. The low ambient metallicity is expected to lower the mass-loss rate by stellar winds. Therefore, it increases the minimum mass to form Wolf-Rayet (WR) stars. Binarity is then expected to be responsible of the formation of a large fraction of WR stars in the Magellanic Clouds. We present here the rationale behind a systematic search for radial velocity variations in a subsample of WR stars both in the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). Some very preliminary results of this study are also presented and discussed." @default.
- W1560761392 created "2016-06-24" @default.
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- W1560761392 date "2001-01-01" @default.
- W1560761392 modified "2023-10-03" @default.
- W1560761392 title "Systematic Search for Wolf-Rayet Binaries in the Magellanic Clouds: Preliminary Results" @default.
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- W1560761392 doi "https://doi.org/10.1007/978-94-015-9723-4_12" @default.
- W1560761392 hasPublicationYear "2001" @default.
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