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dc.contributor.authorGallimore, J.F.
dc.contributor.authorBaum, S.A.
dc.contributor.authorO'Dea, C.P.
dc.contributor.authorPedlar, A.
dc.contributor.authorBrinks, E.
dc.date.accessioned2007-10-23T14:21:13Z
dc.date.available2007-10-23T14:21:13Z
dc.date.issued1999
dc.identifier.citationGallimore , J F , Baum , S A , O'Dea , C P , Pedlar , A & Brinks , E 1999 , ' Neutral Hydrogen (21 Centimeter) Absorption in Seyfert Galaxies: Evidence for Free-Free Absorption and Subkiloparsec Gaseous Disks ' , The Astrophysical journal , vol. 524 , pp. 684-706 .
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 168543
dc.identifier.otherPURE UUID: d8755d36-96ed-470b-9cef-6b30bd34611f
dc.identifier.otherdspace: 2299/969
dc.identifier.otherScopus: 0033589234
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407915
dc.identifier.urihttp://hdl.handle.net/2299/969
dc.descriptionOriginal article can be found at: http://www.journals.uchicago.edu/ApJ/front.html--Copyright American Astronomical Society
dc.description.abstractActive galaxies are thought to be both fueled and obscured by neutral gas removed from the host galaxy and funneled into a central accretion disk. We performed a VLA imaging survey of 21 cm absorption in Seyfert and starburst nuclei to study the neutral gas in the near-nuclear environment. With the exception of NGC 4151, the absorbing gas traces 100 pcÈscale, rotating disks aligned with the outer galaxy disk. These disks appear to be rich in atomic gas relative to nuclear disks in nonactive spirals. We Ðnd no strong evidence for rapid infall or outÑow of neutral hydrogen, but our limits on the mass infall rates are compatible with that required to feed a Seyfert nucleus. Among the galaxies surveyed here, neutral hydrogen absorption traces parsec-scale gas only in NGC 4151. Based on the kinematics of the absorption line, the disk symmetry axis appears to align with the radio jet axis rather than the outer galaxy axis. The most surprising result is that we detect no 21 cm absorption toward the central radio sources of the hidden Seyfert 1 nuclei Mrk 3, Mrk 348, and NGC 1068. Moreover, 21 cm absorption is commonly observed toward extended radio jet structure but appears to avoid central, compact radio sources in Seyfert nuclei. To explain these results, we propose that 21 cm absorption toward the nucleus is suppressed by either free-free absorption, excitation e ects (i.e., enhanced spin temperature), or rapid motion in the obscuring gas. Ironically, the implications of these e ects is that the obscuring disks must be small, typically not larger than a few tens of parsecs.en
dc.language.isoeng
dc.relation.ispartofThe Astrophysical journal
dc.titleNeutral Hydrogen (21 Centimeter) Absorption in Seyfert Galaxies: Evidence for Free-Free Absorption and Subkiloparsec Gaseous Disksen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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