Local dark energy: HST evidence from the vicinity of the M 81/M 82 galaxy group

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dc.creatorChernin, A. D.
dc.creatorKarachentsev, I. D.
dc.creatorKashibadze, O. G.
dc.creatorMakarov, D. I.
dc.creatorTeerikorpi, P.
dc.creatorValtonen, M. J.
dc.creatorDolgachev, V. P.
dc.creatorDomozhilova, L. M.
dc.date2007-06-28
dc.date.accessioned2026-07-07T10:56:30Z
dc.date.available2026-07-07T10:56:30Z
dc.descriptionThe Hubble Space Telescope observations of the nearby galaxy group M 81/M 82 and its vicinity indicate that the expansion outflow around the group is dominated by the antigravity of the dark energy background. The local density of dark energy in the area is estimated to be near the global dark energy density or perhaps exactly equal to it. This conclusion agrees with our previous results for the Local group vicinity and the vicinity of the Cen A/M 83 group.
dc.description17 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/0706.4171
dc.identifierhttp://arxiv.org/abs/0706.4171
dc.identifierAstrophys.50:405-415,2007
dc.identifierdoi:10.1007/s10511-007-0038-2
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186433
dc.subjectAstrophysics
dc.titleLocal dark energy: HST evidence from the vicinity of the M 81/M 82 galaxy group
dc.typetext

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