Molecular Gas in nearby Early-Type Powerful Classical Radio Galaxies

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dc.creatorLeon, Stephane
dc.creatorLim, Jeremy
dc.creatorCombes, Francoise
dc.creatorDinh-V-Trung
dc.date2002-11-13
dc.date.accessioned2026-07-07T02:06:12Z
dc.date.available2026-07-07T02:06:12Z
dc.descriptionWe report a survey for molecular gas in nearby powerful radio galaxies. Eight of the eighteen radio galaxies observed were detected with molecular masses in the range 10^7--10^9 Msun, similar to the same survey we performed towards 3C radio galaxies. The upper limits of molecular gas in the remainder are typically of 10^8 Msun, indicating that very few radiogalaxies have molecular gas reservoir with more than 10^9 Msun.
dc.description2 pages, to appear in Active Galactic Nuclei: from Central Engine to Host Galaxy Abstract Book, meeting held in Meudon, France, July 23-27, 2002, Eds.: S. Collin, F. Combes and I. Shlosman (ASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/0211279
dc.identifierhttp://arxiv.org/abs/astro-ph/0211279
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5338
dc.subjectAstrophysics
dc.titleMolecular Gas in nearby Early-Type Powerful Classical Radio Galaxies
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