Constrained Simulations of the Real Universe: II. Observational Signatures of Intergalactic Gas in the Local Supercluster Region

Preprint

6 September 2001

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0109077

Abstract

We present results of gasdynamics+N-body constrained cosmological simulations of the Local Supercluster region (LSC; about 30/h Mpc around the Virgo cluster), which closely mimic the real Universe within 100 Mpc by imposing constraints from Mark III catalog of galaxy peculiar velocities. The simulations are used to study the properties and possible observational signatures of intergalactic medium in the LSC region. We find that, in agreement with previous unconstrained simulations, about 30% of the gas in this region is in the warm/hot phase at T~10^5-10^7 K, and about 40% in the diffuse phase at T0.05, the column densities of OVI, OVII, and OVIII along a random line of sight near the North Galactic Pole, especially near the supergalactic plane, have a significant probability to be in the range detectable by the current (FUSE,XMM) and future (Constellation-X) instruments. (Abridged)

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Version 1, 2001-09-06, ArXiv
Published version: The Astrophysical Journal, 571 (2), 563.

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