Reference : Hydrodynamic simulations of galaxy formation
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/149278
Hydrodynamic simulations of galaxy formation
English
Thoul, Anne mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie >]
Jul-1995
Dark Matter
AIP Conference Proceedings
AIP Conference Proceedings, Volume 336
437-440
No
No
International
39th Annual October Astrophysics Conference “Dark Matter”
octobre 1994
College Park, Maryland
USA
[en] We have developed an accurate, one-dimensional, spherically symmetric, Lagrangian hydrodynamics/gravity code, designed to study the effects of radiative cooling and photo-ionization on the formation of protogalaxies. We examine the ability of collapsing perturbations to cool within the age of the universe. In contrast to some studies based on order-of-magnitude estimates, we find that cooling arguments alone cannot explain the sharp upper cutoff observed in the galaxy luminosity function. We also look at the effect of a photoionizing background on the formation of low-mass galaxies.
http://hdl.handle.net/2268/149278

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