The very local Hubble flow: Simulating transition from chaos to order

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dc.creatorChernin, A. D.
dc.creatorKarachentsev, I. D.
dc.creatorValtonen, M. J.
dc.creatorDolgachev, V. P.
dc.creatorDomozhilova, L. M.
dc.creatorMakarov, D. I.
dc.date2005-07-15
dc.date.accessioned2026-07-07T02:18:17Z
dc.date.available2026-07-07T02:18:17Z
dc.descriptionThe physical nature of the very local (<3 Mpc) Hubble flow is studied on the basis of the recent high precision observations in the Local Volume. A model including both analytical treatment and computer simulations describes the flow dynamical evolution from a chaotic Little Bang initial state to the present-day state of a quasi-regular expansion. The two major observational parameters of the flow, which are the rate of expansion and the velocity dispersion, find a clear qualitative and quantitative explanation in the model.
dc.descriptionsubmitted to A&A
dc.identifierhttps://arxiv.org/abs/astro-ph/0507364
dc.identifierhttp://arxiv.org/abs/astro-ph/0507364
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9427
dc.subjectAstrophysics
dc.titleThe very local Hubble flow: Simulating transition from chaos to order
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