The DOI matches its Crossref record; 22 of the 22 references it cites were found in a registry or an index.
Virial shocks in galactic haloes?
Open accessAbstract
We investigate the conditions for the existence of an expanding virial shock in the gas falling within a spherical dark matter halo. The shock relies on pressure support by the shock-heated gas behind it. When the radiative cooling is efficient compared with the infall rate, the post-shock gas becomes unstable; it collapses inwards and cannot support the shock. We find for a monatomic gas that the shock is stable when the post-shock pressure and density obey . When expressed in terms of the pre-shock gas properties at radius r it reads as ρrΛ(T)/u3 < 0.0126, where ρ is the gas density, u is the infall velocity and Λ(T) is the cooling function, with the post-shock temperature T∝u2. This result is confirmed by hydrodynamical simulations, using an accurate spheri-symmetric Lagrangian code. When the stability analysis is applied in cosmology, we find that a virial shock does not develop in most haloes that form before z∼ 2, and it never forms in haloes less massive than a few 1011 M⊙. In such haloes, the infalling gas is not heated to the virial temperature until it hits the disc, thus avoiding the cooling-dominated quasi-static contraction phase. The direct collapse of the cold gas into the disc should have non-trivial effects on the star formation rate and on outflows. The soft X-ray produced by the shock-heated gas in the disc is expected to ionize the dense disc environment, and the subsequent recombination would result in a high flux of Lα emission. This may explain both the puzzling low flux of soft X-ray background and the Lα emitters observed at high redshift.
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Citations
Cites
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“…considerations indicate that feedback effects are likely to be important in galaxies as large as ∼ 1011M⊙ and may thus affect the shock stability (e.g. Dekel & Silk 1986; Dekel & Woo 2003, and references therein), it has proven difficult for numerical simulations to reproduce such effects in any…”
BackgroundSelf-citationThe formation and evolution of galaxies within merging dark matter haloes*
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A Universal Angular Momentum Profile for Galactic Halos
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THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROM z = 0-8
Behroozi, P. S., Wechsler, R. H., & Conroy, C. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/770/1/57 · Cited by 2,167
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The physics driving the cosmic star formation history
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Theoretical Challenges in Galaxy Formation
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The Assembly of the First Massive Black Holes
Inayoshi, K., Visbal, E., & Haiman, Z. (2020) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-120419-014455 · Cited by 665
Metadata
- Authors
- Birnboim, Y., & Dekel, A.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2003-10
- Volume
- 345
- Issue
- 1
- Pages
- 349-364
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2122910569
- Cited by
- 1,080
- References
- 22
- FWCI
- 14.30
- Type
- journal article
- Language
- en
- Open access
- bronze
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