A Search for Molecular Gas in Low Luminosity Radio Galaxies

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dc.creatorPrandoni, I.
dc.creatorLaing, R. A.
dc.creatorParma, P.
dc.creatorde Ruiter, H. R.
dc.creatorMontenegro-Montes, F. M.
dc.creatorWilson, T. L.
dc.date2006-08-28
dc.date.accessioned2026-07-07T07:19:26Z
dc.date.available2026-07-07T07:19:26Z
dc.descriptionWe discuss CO spectral line data of a volume-limited sample of 23 nearby (z<0.03) low luminosity radi galaxies, selected from the B2 catalogue. Most of such objects (16/23) have HST imaging. Our aim is to establish the distribution of molecular gas masses in low luminosity radio galaxies, in comparison with other radio source samples, confirm the suggestion that the CO is in ordered rotation, determine its relation to the dust disks observed in these objects with HST and establish targets for future interferometric imaging.
dc.description4 pages, 2 figures. To appear in "From Z-Machines to ALMA: (Sub)millimeter Spectroscopy of Galaxies", ASP Conf. Series, A.J. Baker et al. eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0608577
dc.identifierhttp://arxiv.org/abs/astro-ph/0608577
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/114623
dc.subjectAstrophysics
dc.titleA Search for Molecular Gas in Low Luminosity Radio Galaxies
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