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Hydrodynamic Simulations of Galaxy Formation. II. Photoionization and the Formation of Low-Mass Galaxies

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Thoul, Anne A., Weinberg, David H.·1996·The Astrophysical Journal

Abstract

Photoionization by the high-redshift ultraviolet radiation background heats low- density gas before it falls into dark matter potential wells, and it eliminates the neutral hydrogen and singly ionized helium that dominate cooling of primordial gas at temperatures of 10^4^-10^5^ K. We investigate the influence of photoionization on galaxy formation using high-resolution simulations with a one-dimensional, spherically symmetric, Lagrangian hydrodynamics/gravity code. We find that the presence of a photoionizing background suppresses the formation of galaxies with circular velocities v_circ_ <~ 30 km s^-1^ and substantially reduces the mass of cooled baryons in systems with circular velocities up to v_circ_ ~ 50 km s^-1^. Above v_circ_ ~ 75 km s^-1^, photoionization has no significant effect. Photoionization exerts its influence primarily by heating gas before collapse; the elimination of line cooling processes is less important. We discuss the implications of these results for hierarchical theories of galaxy formation.

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Metadata

Authors
Thoul, A. A., & Weinberg, D. H.
Venue
The Astrophysical Journal
Published
1996-07
Volume
465
Pages
608
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2046076359
Cited by
457
References
0
FWCI
11.24
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Hydrodynamic Simulations of Galaxy Formation. II. Photoionization and the Formation of Low-Mass Galaxies. https://app.cochat.ai/papers/10.1086/177446
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Thoul, A. A., & Weinberg, D. H. (1996). Hydrodynamic Simulations of Galaxy Formation. II. Photoionization and the Formation of Low-Mass Galaxies. The Astrophysical Journal. https://doi.org/10.1086/177446

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