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Ly�� blobs as an observational signature of cold accretion streams into galaxies

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Dijkstra, Mark, Loeb, Abraham·2009·Monthly Notices of the Royal Astronomical Society

Abstract

Recent hydrodynamic simulations of galaxy formation reveal streams of cold (T∼ 104 K) gas flowing into the centres of dark matter haloes as massive as 1012−13.5 M⊙ at redshifts z∼ 1–3. In this paper, we show that if ≳20 per cent of the gravitational binding energy of the gas is radiated away then the simulated cold flows are spatially extended Lyα sources with luminosities, Lyα linewidths and number densities that are comparable to those of observed Lyα blobs. Furthermore, the filamentary structure of the cold flows can explain the wide range of observed Lyα blob morphologies. Since the most massive haloes form in dense environments, the association of Lyα blobs with overdense regions arise naturally. We argue that Lyα blobs – even those which are clearly associated with starburst galaxies or quasars – provide direct observational support for the cold accretion mode of galaxies. We discuss various testable predictions of this association.

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Crossref · 10.1111/j.1365-2966.2009.15533.x

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Metadata

Authors
Dijkstra, M., & Loeb, A.
Venue
Monthly Notices of the Royal Astronomical Society
Published
2009-12-01
Volume
400
Issue
2
Pages
1109-1120
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2115601889
Cited by
188
References
1
FWCI
8.22
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Ly�� blobs as an observational signature of cold accretion streams into galaxies. https://app.cochat.ai/papers/10.1111/j.1365-2966.2009.15533.x
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Dijkstra, M., & Loeb, A. (2009). Ly�� blobs as an observational signature of cold accretion streams into galaxies. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2009.15533.x

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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