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Properties of galax...
Properties of galaxy haloes in clusters and voids
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Antonuccio-Delogu, V. (författare)
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Becciani, U. (författare)
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van Kampen, E. (författare)
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Pagliaro, A. (författare)
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- Romeo, Alessandro, 1961 (författare)
- Chalmers tekniska högskola,Chalmers University of Technology
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et al., (författare)
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(creator_code:org_t)
- 2002
- 2002
- Engelska.
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Ingår i: Monthly Notices of the Royal Astronomical Society. - 0035-8711 .- 1365-2966. ; 332:1, s. 7-20
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Abstract
Ämnesord
Stäng
- We use the results of a high-resolution N -body simulation to investigate the role of the environment on the formation and evolution of galaxy-sized haloes. Starting from a set of constrained initial conditions, we have produced a final configuration hosting a double cluster in one octant and a large void extending over two octants of the simulation box. In this paper we concentrate on gravitationally bound galaxy-sized haloes extracted from these two regions and from a third region hosting a single, relaxed cluster without substructure. Exploiting the high mass resolution of our simulation (m body =2.1×109 h -1 Msolar ), we construct halo samples probing more than two decades in mass, starting from a rather small mass threshold: 5×1010 h -1 Msolar =34.2r 0 , where r 0 is the core radius of the TIS solution). We do, however, find a dependence of this relationship on the environment, like for the P (lambda ) statistics. These facts hint at a possible role of tidal fields in determining the statistical properties of haloes.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
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- ref (ämneskategori)
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