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Are cold flows detectable with metal absorption lines?

Abstract:: [Abridged] Cold gas flowing within the "cosmic web" is believed to be an important source of fuel for star formation at high redshift. However, the presence of such filamentary gas has never been observationally confirmed. In this work, we investigate in detail whether such cold gas is detectable using low-ionisation metal absorption lines, such as CII \lambda1334 as this technique has a proven observational record for detecting gaseous structures. Using a large statistical sample of galaxies...
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Publication status:: Published

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APA Style

Kimm, T., Slyz, A., Devriendt, J., & Pichon, C. (2010). Are cold flows detectable with metal absorption lines? Monthly Notices of the Royal Astronomical Society, 413(1), L51–L55.

MLA Style

Kimm, T., et al. “Are Cold Flows Detectable with Metal Absorption Lines?” Monthly Notices of the Royal Astronomical Society, vol. 413, no. 1, 2010, pp. L51–L55.

Chicago Style

Kimm, T, A Slyz, J Devriendt, and C Pichon. 2010. “Are Cold Flows Detectable with Metal Absorption Lines?” Monthly Notices of the Royal Astronomical Society 413 (1): L51–L55.
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Publisher copy:: 10.1111/j.1745-3933.2011.01031.x

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+ Kimm, T More by this author

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+ Slyz, A More by this author

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+ Devriendt, J More by this author

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+ Pichon, C More by this author

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Bibliographic Details

Journal:: Monthly Notices of the Royal Astronomical Society
Volume:: 413
Issue:: 1
Pages:: L51-L55
Publication date:: 2010-11-30
DOI:: 10.1111/j.1745-3933.2011.01031.x
ISSN:: 0035-8711

Item Description

Language:: English
Keywords:: astro-ph.CO
Pubs id:: pubs:205695
UUID:: uuid:3c1a101e-a73f-4d5d-ba64-d0be8dcc1234
Local pid:: pubs:205695
Source identifiers:: 205695
Deposit date:: 2012-12-19

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Copyright date:: 2010
Notes:: MNRAS Letters in press

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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