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- W2479968213 abstract "Stellar emission and absorption lines are routinely observed in galaxies at redshifts up to 5 with spectrographs on 8-10m class telescopes. While the overall spectra are well understood and have been successfully modeled using empirical and theoretical libraries, some challenges remain. Three issues are discussed: determining abundances using stellar and interstellar spectral lines, understanding the origin of the strong, stellar He II 1640 line, and gauging the influence of stellar Lyman-alpha on the combined stellar+nebular profile. All three issues can be tackled with recently created theoretical stellar libraries for hot stars which take into account the radiation-hydrodynamics of stellar winds." @default.
- W2479968213 created "2016-08-23" @default.
- W2479968213 creator A5042936481 @default.
- W2479968213 date "2013-12-09" @default.
- W2479968213 modified "2023-09-27" @default.
- W2479968213 title "Stellar Spectral Signatures in High-Redshift Galaxies" @default.
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- W2479968213 hasPublicationYear "2013" @default.
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