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<ri:Resource created="2008-01-23T20:52:42Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Classification of planetary nebulae</title><shortName>J/A+A/475/217</shortName><identifier>ivo://CDS.VizieR/J/A+A/475/217</identifier><altIdentifier>doi:10.26093/cds/vizier.34750217</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Quireza C.</name></creator><creator><name>Rocha-Pinto H.J.</name></creator><creator><name>Maciel W.J.</name></creator><date role="Updated">2017-06-20T13:16:27Z</date><date role="Created">2008-01-23T20:52:42Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>planetary-nebulae</subject><subject>chemical-abundances</subject><description>In this paper we present a re-analysis of the criteria used to characterize the Peimbert classes I, IIa, IIb, III and IV, through a statistical study of a large sample of planetary nebulae previously classified according to these groups. In the original classification, it is usual to find planetary nebulae that cannot be associated with a single type; these most likely have dubious classifications into two or three types. Statistical methods can greatly contribute in providing a better characterization of planetary nebulae groups. We use the Bayes Theorem to calculate the posterior probabilities for an object to be member of each of the types I, IIa, IIb, III and IV. This calculation is particularly important for planetary nebulae that are ambiguously classified in the traditional method. The posterior probabilities are defined from the probability density function of classificatory parameters of a well-defined sample, composed only by planetary nebulae unambiguously fitted into the Peimbert types. Because the probabilities depend on the available observational data, they are conditional probabilities, and, as new observational data are added to the sample, the classification of the nebula can be improved, to take into account this new information. This method differs from the original classificatory scheme, because it provides a quantitative result of the representativity of the object within its group. Also, through the use of marginal distributions it is possible to extend the Peimbert classification even to those objects for which only a few classificatory parameters are known.</description><source format="bibcode">2007A&amp;A...475..217Q</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/475/217</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/V/84">V/84 : Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker+, 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/127">V/127 : MASH Catalog of Planetary Nebulae (Parker+ 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planetary nebulae</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Planetary nebula main designation (Common name)</description><ucd>meta.id;phys.atmol.configuration;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>PNG</name><description>Designation of the Galactic Planetary Nebula</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>He/H</name><description>? Helium over hydrogen abundance ratio by number</description><ucd>phys.abund.Y;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_He/H</name><description>[:] Note about the He/H abundance ratio (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>r_He/H</name><description>Reference of the He/H abundance ratio</description><ucd>meta.ref;phys.abund.Y</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>lg(O/H)+12</name><description>? Oxygen over hydrogen abundance ratio by number</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_lg(O/H)+12</name><description>Reference of the O/H abundance ratio</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>lg(N/H)+12</name><description>? Nitrogen over hydrogen abundance ratio by number</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_lg(N/H)+12</name><description>Reference of the N/H abundance ratio</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>lg(N/O)</name><description>? 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Absolute value of the height in relation to the Galactic plane</description><unit>kpc</unit><ucd>pos.cartesian.z;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>VLSR</name><description>? Radial velocity relative to the Local Sandard of Rest (2)</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs(DV)</name><description>? Absolute value of the peculiar velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Theta</name><description>? Angular diameter of the planetary nebula</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_Theta</name><description>Reference of the angular diameter</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>S5GHz</name><description>? 5GHz (6cm) radio flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.3-6GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_S5GHz</name><description>? Reference of the 5 GHz flux density</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Type</name><description>Classification according to the Peimbert's types</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>p(typeI)</name><description>Posterior probability for the membership of each object to the type I group</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(typeIIa)</name><description>Posterior probability for the membership of each object to the type IIa group</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(typeIIb)</name><description>Posterior probability for the membership of each object to the type IIb group</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(typeIII)</name><description>Posterior probability for the membership of each object to the type III group</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(typeIV)</name><description>Posterior probability for the membership of each object to the type IV group</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pre-class</name><description>Previous classification (as in column "Type" of Table 1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>Post-class</name><description>Posterior classification</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>_RA</name><description>Computed Right Ascension for Equinox: J2000</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Computed Declination for Equinox: J2000</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/A+A/475/217/refs</name><description>References</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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