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- W2076759974 abstract "We present a simple method for tracing the spatial distribution and predicting the physical properties of the Warm-Hot Intergalactic Medium (WHIM), from the map of galaxy light in the Local Universe. Under the assumption that biasing is local and monotonic we map the ∼2 h -1 Mpc smoothed density field of galaxy light into the mass-density field, from which we infer the spatial distribution of the WHIM in the Local Supercluster. Taking into account the scatter in the WHIM density-temperature and density-metallicity relation, extracted from the z = 0 outputs of high-resolution and large-box-size hydrodynamical cosmological simulations, we are able to quantify the probability of detecting WHIM signatures in the form of absorption features in the X-ray spectra, along arbitrary directions in the sky. To illustrate the usefulness of this semi-analytical method we focus on the WHIM properties in the Virgo cluster region." @default.
- W2076759974 created "2016-06-24" @default.
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- W2076759974 date "2005-07-01" @default.
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- W2076759974 title "Tracing the warm-hot intergalactic medium in the local Universe" @default.
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- W2076759974 doi "https://doi.org/10.1111/j.1365-2966.2005.09097.x" @default.
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