Gas/Star Offsets in Tidal Tails

dc.creatorMihos, Chris
dc.date2000-08-09
dc.date.accessioned2026-07-07T01:54:53Z
dc.date.available2026-07-07T01:54:53Z
dc.descriptionWe use numerical simulations to study the development of gas/star offsets in the tidal tails of merging galaxies. These offsets are shown to be a natural consequence of the radially extended HI spatial distribution in disk galaxies, coupled with internal dissipation in the gaseous component driven by the interaction. This mechanism explains the observed gas/star offsets in interacting galaxies without invoking interactions with a hot (unseen) gaseous component.
dc.description2 pages, 1 Postscript figure, uses newpasp.sty. To appear in the conference proceedings of "Gas and Galaxy Evolution"
dc.identifierhttps://arxiv.org/abs/astro-ph/0008153
dc.identifierhttp://arxiv.org/abs/astro-ph/0008153
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1465
dc.subjectAstrophysics
dc.titleGas/Star Offsets in Tidal Tails
dc.typetext

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