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dc.contributor.authorUsero, A.
dc.contributor.authorGarcia-Burillo, S.
dc.contributor.authorFuente, A.
dc.contributor.authorMartin-Pintado, J.
dc.date.accessioned2008-02-01T11:43:31Z
dc.date.available2008-02-01T11:43:31Z
dc.date.issued2004
dc.identifier.citationUsero , A , Garcia-Burillo , S , Fuente , A & Martin-Pintado , J 2004 , XDR Chemistry in the Circumnuclear Disk of NGC 1068 . in In: The Neutral ISM in Starburst Galaxies - ASP Conf Series 320 . Astronomical Society of the Pacific , pp. 273-6 .
dc.identifier.isbn1-58381-182-6
dc.identifier.isbn978-1-58381-255-6
dc.identifier.otherdspace: 2299/1520
dc.identifier.urihttp://hdl.handle.net/2299/1520
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/309.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe have studied the feedback in°uence that the central engine of the Seyfert 2 galaxy NGC 1068 may have on the chemistry of the 200 pc circumnuclear gas disk (CND). With this purpose, we have conducted a multispecies/ multi-transition survey of molecular gas in the CND of NGC 1068 using the IRAM 30m telescope. Abundances of several molecular species have been estimated, including HCN, CN, CS, HCO+, SiO and HOC+. We report on the detection of signi¯cant SiO emission in this galaxy, as well as on the ¯rst extragalactic detection of the active radical HOC+. We conclude that the chemistry of the molecular gas reservoir in the CND can be best explained in the framework of X-ray Dominated Region (XDR) models.en
dc.format.extent166130
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: The Neutral ISM in Starburst Galaxies - ASP Conf Series 320
dc.titleXDR Chemistry in the Circumnuclear Disk of NGC 1068en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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