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Detectability of cold streams into high-redshift galaxies by absorption lines

  • Published:2012-07-03 Issue:3 Volume:424 Page:2292-2315
  • ISSN:0035-8711
  • Container-title:Monthly Notices of the Royal Astronomical Society
  • language:en
  • Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Goerdt Tobias1,Dekel Avishai2,Sternberg Amiel3,Gnat Orly2,Ceverino Daniel1

Affiliation:

1. Departamento de Física Teórica; Universidad Autónoma de Madrid; 28049; Madrid; Spain

2. Racah Institute of Physics; The Hebrew University; Jerusalem; 91904; Israel

3. The Raymond and Beverly Sackler School of Physics and Astronomy; Tel Aviv University; Tel Aviv; 69978; Israel

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. Evolution of cold streams in hot gaseous haloes;Monthly Notices of the Royal Astronomical Society;2024-03-18

2. Dissecting cosmological filaments at high redshifts: emergence of spaghetti-type flow inside DM haloes;Monthly Notices of the Royal Astronomical Society;2023-12-21

3. The structure and dynamics of massive high-z cosmic-web filaments: three radial zones in filament cross-sections;Monthly Notices of the Royal Astronomical Society;2023-12-07

4. Ly α blobs from cold streams undergoing Kelvin–Helmholtz instabilities;Monthly Notices of the Royal Astronomical Society;2020-09-02

5. Detecting the cosmic web: Lyα emission from simulated filaments at z = 3;Monthly Notices of the Royal Astronomical Society;2020-04-21
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