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dc.contributor.authorGarcia-Burillo, S.
dc.contributor.authorFuente, A.
dc.contributor.authorUsero, A.
dc.contributor.authorMartin-Pintado, J.
dc.date.accessioned2008-02-01T11:43:32Z
dc.date.available2008-02-01T11:43:32Z
dc.date.issued2004
dc.identifier.citationGarcia-Burillo , S , Fuente , A , Usero , A & Martin-Pintado , J 2004 , Chemistry of Molecular Gas in Starbursts and AGN . in In: The Neutral ISM in Starburst Galaxies - ASP Conf Series 320 . Astronomical Society of the Pacific , pp. 15-18 .
dc.identifier.isbn1-58381-182-6
dc.identifier.isbn978-1-58381-255-6
dc.identifier.otherPURE: 147849
dc.identifier.otherPURE UUID: b3b1712d-7f9e-434e-bf7f-7b3f36005da2
dc.identifier.otherdspace: 2299/1521
dc.identifier.urihttp://hdl.handle.net/2299/1521
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/309.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe present the main results of an extragalactic survey aiming to study the chemistry of molecular gas in a limited sample of starburst galaxies (SB) and AGN hosts. Observations have been carried out with the IRAM 30m telescope and the Plateau de Bure Interferometer (PdBI). The high resolution/sensitivity of the PdBI has made possible to obtain high quality images of the galaxies using specific molecular gas tracers of Shock Chemistry, Photon Dominated Regions (PDR) and X-ray Dominated Regions (XDR). The occurrence of large-scale shocks and the propagation of PDR in starbursts can be studied. We also discuss the onset of XDR chemistry in AGN.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: The Neutral ISM in Starburst Galaxies - ASP Conf Series 320
dc.titleChemistry of Molecular Gas in Starbursts and AGNen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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