New Dwarf Galaxies in the IC342/Maffei Group

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dc.creatorHuchtmeier, W. K.
dc.creatorKarachentsev, I. D.
dc.creatorKarachentseva, V. E.
dc.date1999-07-26
dc.date.accessioned2026-07-07T02:32:38Z
dc.date.available2026-07-07T02:32:38Z
dc.descriptionWe report detection of HI-emission from three 'new' dwarf galaxies Perseus A, Perseus B, and Camelopardalis D in the IC342/Maffei group of galaxies and of Draco A. The actual number of (probable) members of this group increases to 19 galaxies. Its velocity dispersion is 87 km/s. With a distance of 2.2+-0.5 Mpc this group is the nearest to the Local Group and might have considerable dynamical influence on the Local Group.
dc.description4 pages, 2 figures, uses paspconf.sty to be published in IAU Coll. 174 "Small Galaxy Groups" M. Valtonen, C. Flynn (eds.) pasp conf.series
dc.identifierhttps://arxiv.org/abs/astro-ph/9907344
dc.identifierhttp://arxiv.org/abs/astro-ph/9907344
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14531
dc.subjectAstrophysics
dc.titleNew Dwarf Galaxies in the IC342/Maffei Group
dc.typetext

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