QUENCHED COLD ACCRETION OF A LARGE-SCALE METAL-POOR FILAMENT DUE TO VIRIAL SHOCKING IN THE HALO OF A MASSIVEz= 0.7 GALAXY-Reference-Cited by-同舟云学术

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QUENCHED COLD ACCRETION OF A LARGE-SCALE METAL-POOR FILAMENT DUE TO VIRIAL SHOCKING IN THE HALO OF A MASSIVEz= 0.7 GALAXY

Published:2012-11-07 Issue:1 Volume:760 Page:68
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Churchill Christopher W.,Kacprzak Glenn G.,Steidel Charles C.,Spitler Lee R.,Holtzman Jon,Nielsen Nikole M.,Trujillo-Gomez Sebastian

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/760/i=1/a=68/pdf

Reference103 articles.

1. The Morphologies of Distant Galaxies. II. Classifications from the Hubble Space Telescope Medium Deep Survey

2. High-metallicity, photoionized gas in intergalactic large-scale filaments

3. Erratum: High-metallicity, photoionized gas in intergalactic large-scale filaments

4. The Chemical Composition of the Sun

5. The Hubble Space Telescope quasar absorption line key project. I - First observational results, including Lyman-alpha and Lyman-limit systems

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