J/MNRAS/409/881ivo://CDS.VizieR/J/MNRAS/409/881doi:10.26093/cds/vizier.74090881CDSPhillips J.P.Cuesta L.C.Ramos-Larios G.2024-07-12T20:14:59Z2011-06-07T13:50:11ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frplanetary-nebulaespectroscopyNGC 7009 is a fascinating example of a high-excitation, elliptical planetary nebula (PN) containing circumnebular rings, and FLIERs and jets along the major axis. We present visual spectroscopy along multiple position angles through the nucleus, taken with the Observatorio Astronomico Nacional (Mexico); mid-infrared (MIR) spectroscopy and imaging acquired using the Infrared Space Observatory (ISO) and Spitzer Space Telescope (SST), and narrow-band imaging obtained using the Hubble Space Telescope (HST).2010MNRAS.409..881Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/409/881CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/409/881https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/409/881http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/409/881https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/409/881https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/409/881http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/409/881GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/MNRAS/409/881/table1Line intensities for six sectors of the envelope in NGC 7009recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIon namephys.atmol.ionStagecharlambdaWavelength0.1nmem.wldoubleF(T)? Line intensity for total emission (T) (1)spect.line.intensitydoublenullablee_F(T)? rms uncertainty on FTstat.errordoublenullableF(I)? Line intensity for sector I (nucleus) (1)spect.line.intensitydoublenullablee_F(I)? rms uncertainty on FIstat.errordoublenullableF(II)? Line intensity for sector II (bright elliptical inner rim structure) (1)spect.line.intensitydoublenullablee_F(II)? rms uncertainty on FIIstat.errordoublenullableF(III)? Line intensity for sector III (fainter, more spherical enveloping shell) (1)spect.line.intensitydoublenullablee_F(III)? rms uncertainty on FIIIstat.errordoublenullableF(IV)? Line intensity for sector IV (jet-like feature) (1)spect.line.intensitydoublenullablee_F(IV)? rms uncertainty on FIVstat.errordoublenullableF(V)? Line intensity for sector V (ansae) (1)spect.line.intensitydoublenullablee_F(V)? rms uncertainty on FVstat.errordoublenullableF(VI)? Line intensity for sector VI (external halo) (1)spect.line.intensitydoublenullablee_F(VI)? rms uncertainty on FVIstat.errordoublenullable