Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2530
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dc.contributor.authorZhao, J.H.-
dc.contributor.authorGoss, W.M.-
dc.contributor.authorUlvestad, J.S.-
dc.contributor.authorAnantharamaiah, K.R.-
dc.date.accessioned2007-05-29T10:55:03Z-
dc.date.available2007-05-29T10:55:03Z-
dc.date.issued2001-
dc.identifier.citationASP Conference Series, 2001, Vol.240, p404en
dc.identifier.isbn1-58381-077-3-
dc.identifier.urihttp://hdl.handle.net/2289/2530-
dc.descriptionRestricted Access. Gas and Galaxy Evolution, ASP Conference Proceedings, Vol. 240. Eds. John E. Hibbard, Michael Rupen, and Jacqueline H. van Gorkom. San Francisco: Astronomical Society of the Pacific, 2001,en
dc.description.abstractWe report on new VLA H53α line observations at 7 mm of the nuclear region of NGC 253 with an angular resolution of 1'' (15 pc at a distance of 3 Mpc) and a velocity resolution of 44 km s-1. An ionized component with a peculiar velocity VHel~ 400 km s-1 is detected at a position 0.3'' NE of the continuum peak. The kinematics in the nuclear region clearly show a counter-rotating circumnuclear disk, confirming the earlier H92α result of Anantharamaiah & Goss (1996).en
dc.format.extent105837 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2001ASPC..240..404Zen
dc.rights2001 Astronomical Society of the Pacificen
dc.titleHigh velocity ionized component - A counter-rotating circumnuclear disk in NGC 253en
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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