4.7 Article

Faint resonantly scattered Lyα emission from the absorption troughs of damped Lyα systems at z ∼ 3

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1111/j.1745-3933.2010.01004.x

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line: profiles; radiative transfer; galaxies: dwarf; galaxies: formation; galaxies: high-redshift; quasars: absorption lines

资金

  1. STFC [ST/G00269X/1] Funding Source: UKRI
  2. Science and Technology Facilities Council [ST/G00269X/1, ST/H00243X/1] Funding Source: researchfish

向作者/读者索取更多资源

We demonstrate that the Ly alpha emission in the absorption troughs of a large sample of stacked damped Ly alpha absorption systems (DLAS) presented by Rahmani et al. is consistent with the spectral profiles and luminosities of a recently detected population of faint Ly alpha emitters at z similar to 3. This result supports the suggestion that the faint emitters are to be identified with the host galaxies of DLAS at these redshifts.

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