The HI fine structure of HVC187 near NGC3783, gas in the leading bridge of the Magellanic System

dc.creatorWakker, B. P.
dc.creatorSavage, B. D.
dc.creatorOosterloo, T. A.
dc.creatorPutman, M. E.
dc.date1998-11-16
dc.date.accessioned2026-07-07T02:29:08Z
dc.date.available2026-07-07T02:29:08Z
dc.descriptionWe present an analysis of high-resolution HI data of one of the cores of HVC187 Wakker & van Woerden 1991), HVC287+22+240. Structure is present down to the lowest-measurable scale (~1 arcmin) and several concentrations appear to be unresolved. Most of the cores seen at low resolution break up into smaller subcores at higher resolution. The typical volume density and pressure are estimated to be ~30/R/D(kpc) cm^{-3} and ~18000/R/D(kpc) K cm^{-3}, respectively, where R is the resolution in arcmin and D(kpc) the unknown distance in kpc.
dc.description5 pages; LaTeX; to be published in: Proceedings of the 3rd Stromlo Symposium, eds. B.K. Gibson, T.S. Axelrod and M.E. Putman (ASP Conf. Ser.)
dc.identifierhttps://arxiv.org/abs/astro-ph/9811253
dc.identifierhttp://arxiv.org/abs/astro-ph/9811253
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13351
dc.subjectAstrophysics
dc.titleThe HI fine structure of HVC187 near NGC3783, gas in the leading bridge of the Magellanic System
dc.typetext

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