Molecular clouds in cooling flow cluster of galaxies

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dc.creatorGrenacher, L.
dc.creatorJetzer, Ph.
dc.creatorPuy, D.
dc.date1999-11-11
dc.date.accessioned2026-07-07T02:34:21Z
dc.date.available2026-07-07T02:34:21Z
dc.descriptionIn many clusters of galaxies there is evidence for cooling flow in the central regions. A possibility is that a fraction of the gas forms cold molecular clouds. We investigate the minimum temperature which can be reached by clouds in cooling flows by computing the cooling function due to H2, HD and CO molecules. As an example, we determine the minimum temperature achievable by clouds in the cooling flow of PKS 0745-191.
dc.descriptionPoster presented for the IGRAP International Conference "Clustering at high redshifts", Marseille (France) June 29th-July 2nd, 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/9911203
dc.identifierhttp://arxiv.org/abs/astro-ph/9911203
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15211
dc.subjectAstrophysics
dc.titleMolecular clouds in cooling flow cluster of galaxies
dc.typetext

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