Ly α properties of simulated galaxies in overdense regions: effects of galactic winds at $z \gtrsim 6$-Reference-Cited by-同舟云学术

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Ly α properties of simulated galaxies in overdense regions: effects of galactic winds at $z \gtrsim 6$

Published:2019-01-28 Issue:4 Volume:484 Page:4601-4618
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Sadoun Raphael¹²,Romano-Díaz Emilio³,Shlosman Isaac¹⁴^ORCID,Zheng Zheng²

Affiliation:

1. Department of Earth and Space Science, Graduate School of Science, Osaka University, Osaka 560-0043, Japan

2. Department of Physics & Astronomy, University of Utah, Salt Lake City, UT 84112-0830, USA

3. Argelander Institut fuer Astronomie, Auf dem Haegel 71, D-53121 Bonn, Germany

4. Department of Physics & Astronomy, University of Kentucky, Lexington, KY 40506-0055, USA

Funder

Japan Society for the Promotion of Science

Deutsche Forschungsgemeinschaft

National Science Foundation

National Aeronautics and Space Administration

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/484/4/4601/27765766/stz297.pdf

Reference93 articles.

1. Singly Peaked Asymmetric Ly from Starburst Galaxies

2. On the detectability of Lyα emission in star forming galaxies

3. The impact of Lyman-α radiative transfer on large-scale clustering in the Illustris simulation

4. Path integral methods for primordial density perturbations - Sampling of constrained Gaussian random fields

5. UV-CONTINUUM SLOPES ATz∼ 4-7 FROM THE HUDF09+ERS+CANDELS OBSERVATIONS: DISCOVERY OF A WELL-DEFINED UV COLOR-MAGNITUDE RELATIONSHIP FORz⩾ 4 STAR-FORMING GALAXIES

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1. MAMMOTH-Subaru. III. Lyα Halo Identified by Stacking ∼3300 Lyα Emitters at z = 2.2–2.3;The Astrophysical Journal;2024-01-01

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 Ly α, C iv, and He iinebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity atz = 4.5;Monthly Notices of the Royal Astronomical Society;2023-02-23

4. The Magellan M2FS Spectroscopic Survey of High-z Galaxies: Lyα Emitters at z ≈ 6.6 and the Evolution of Lyα Luminosity Function over z ≈ 5.7–6.6;The Astrophysical Journal;2022-02-01

5. SILVERRUSH. IX. Lyα Intensity Mapping with Star-forming Galaxies at z = 5.7 and 6.6: A Possible Detection of Extended Lyα Emission at ≳100 Comoving Kiloparsecs around and beyond the Virial-radius Scale of Galaxy Dark Matter Halos;The Astrophysical Journal;2021-07-01

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