Study of ISM tracers in galaxies

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dc.creatorCasasola, V.
dc.creatorPiovan, L.
dc.creatorGalletta, G.
dc.creatorBettoni, D.
dc.creatorMerlin, E.
dc.date2006-12-05
dc.date.accessioned2026-07-07T07:31:05Z
dc.date.available2026-07-07T07:31:05Z
dc.descriptionWe collected data for two samples of normal and interacting galaxies for a total of 2953 galaxies having fluxes in one or more of the following wavebands: FIR, 21 cm line, CO(1-0) lines and soft X-ray. The large set of data obtained allowed us to revisit some of the already known relations between the different tracers of the interstellar medium (ISM), such as the link between the FIR flux and the CO line emission, the relation between X-ray emission and the blue or FIR luminosity. The relation lacking from observations for early-type galaxies has been discussed and explained in detail in the frame of a suitable theoretical model, obtained by coupling chemo-dynamical N-body simulations with a dusty spectrophotometric code of population synthesis.
dc.description2 pages, o appear in the Proceedings of the Conf. "From Stars to Galaxies: Building the Pieces to Build Up the Universe", Vallenari et al. eds., ASP Conf. Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0612131
dc.identifierhttp://arxiv.org/abs/astro-ph/0612131
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118626
dc.subjectAstrophysics
dc.titleStudy of ISM tracers in galaxies
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