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The origin of the hot metal-poor gas in NGC 1291. Testing the hypothesis of gas dynamics as the cause of the gas heating

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dc.contributor.authorPerez, I
dc.contributor.authorFreeman, Kenneth
dc.date.accessioned2015-12-07T22:33:30Z
dc.date.issued2006
dc.date.updated2015-12-07T10:32:54Z
dc.description.abstractIn this paper we test the idea that the low-metallicity hot gas in the centre of NGC 1291 is heated via a dynamical process. In this scenario, the gas from the outer gas-rich ring loses energy through bar-driven shocks and falls to the centre. Heating of
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/23302
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Energy dissipation; Gas dynamics; Gas heating; Kinematics; Solar energy; Spectroscopy; Thermal effects; Velocity measurement; X rays; Galaxies: ISM; Galaxies: kinematics and dynamics; Galaxies: structure; Galaxy: abundances; X-rays: galaxies; Galaxies Galaxies: ISM; Galaxies: kinematics and dynamics; Galaxies: structure; Galaxy: abundances; X-rays: galaxies
dc.titleThe origin of the hot metal-poor gas in NGC 1291. Testing the hypothesis of gas dynamics as the cause of the gas heating
dc.typeJournal article
local.bibliographicCitation.lastpage169
local.bibliographicCitation.startpage165
local.contributor.affiliationPerez, I, University of Groningen
local.contributor.affiliationFreeman, Kenneth, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidFreeman, Kenneth, u7000399
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4114753xPUB26
local.identifier.citationvolume454
local.identifier.doi10.1051/0004-6361:20052687
local.identifier.scopusID2-s2.0-33746375663
local.type.statusPublished Version

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