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• W2132567745 abstract "In order to study the origin of the strong Lyα emission of high-redshift starburst galaxies we observed and modeled the rest-frame UV spectrum and the Lyα emission of the galaxy FDF-4691 (rest-frame = 103 Å). The observations show that FDF-4691 is a young starburst galaxy with a (for this redshift) typical metallicity. The broad, double-peaked profile of the Lyα emission line can be explained assuming a highly turbulent emission region in the inner part of the starburst galaxy, and a surrounding extended shell of low-density neutral gas with a normal dust/gas ratio and with Galactic dust properties. The detection of the Lyα emission line is explained by the intrinsic broad Lyα emission and a low HI column density of the neutral shell. A low dust/gas ratio in the neutral shell is not needed to explain the strong Lyα line." @default.
• W2132567745 created "2016-06-24" @default.
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• W2132567745 date "2004-02-27" @default.
• W2132567745 modified "2023-09-23" @default.
• W2132567745 title "The nature of the Ly$mathsf{alpha}$-emission region of FDF-4691" @default.
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• W2132567745 doi "https://doi.org/10.1051/0004-6361:20040015" @default.
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