XDR Chemistry in the Circumnuclear Disk of NGC 1068

dc.creatorUsero, A.
dc.creatorGarcia-Burillo, S.
dc.creatorFuente, A.
dc.creatorMartin-Pintado, J.
dc.date2003-10-28
dc.date.accessioned2026-07-07T02:10:53Z
dc.date.available2026-07-07T02:10:53Z
dc.descriptionWe have studied the feedback influence 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 multi-species/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 significant SiO emission in this galaxy, as well as on the first 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-rays Dominated Regions (XDR) models.
dc.description2 pages, 1 figure; poster presented at "The Neutral ISM in Starburst Galaxies", workshop held in Marstrand (Sweden), June 23-27, 2003; to be published in ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0310783
dc.identifierhttp://arxiv.org/abs/astro-ph/0310783
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6887
dc.subjectAstrophysics
dc.titleXDR Chemistry in the Circumnuclear Disk of NGC 1068
dc.typetext

Files

Collections