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- W2330542632 abstract "Determining the precise value of the tangential component of the velocity of M31 is a non trivial astrophysical issue, that relies on complicated modeling. This has recently lead to con- flicting estimates, obtained by several groups that used different methodologies and assump- tions. This letter addresses the issue by computing a Bayesian posterior distribution function of this quantity, in order to measure the compatibility of those estimates with LambdaCDM. This is achieved using an ensemble of local group (LG) look-alikes collected from a set of Con- strained Simulations (CSs) of the local Universe, and a standard unconstrained LambdaCDM. The latter allows us to build a control sample of LG-like pairs and to single out the influence of the environment in our results. We find that neither estimate is at odds with LambdaCDM; how- ever, whereas CSs favour higher values of vtan , the reverse is true for estimates based on LG samples gathered from unconstrained simulations, overlooking the environmental element" @default.
- W2330542632 created "2016-06-24" @default.
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- W2330542632 date "2016-04-03" @default.
- W2330542632 modified "2023-10-02" @default.
- W2330542632 title "The tangential velocity of M31: CLUES from constrained simulations" @default.
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- W2330542632 doi "https://doi.org/10.1093/mnrasl/slw059" @default.
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