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<ri:Resource created="2020-05-14T08:37:37Z" 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>Properties of BAL quasars</title><shortName>J/MNRAS/469/3163</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/469/3163</identifier><altIdentifier>doi:10.26093/cds/vizier.74693163</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>McGraw S.M.</name></creator><creator><name>Brandt W.N.</name></creator><creator><name>Grier C.J.</name></creator><creator><name>Filiz Ak N.</name></creator><creator><name>Hall P.B.,Schneider D.P.</name></creator><creator><name>Anderson S.F.</name></creator><creator><name>Green P.J.</name></creator><creator><name>Hutchinson T.A.</name></creator><creator><name>Macleod C.L.,Vivek M.</name></creator><date role="Updated">2024-08-17T20:19:17Z</date><date role="Created">2020-05-14T08:37:37Z</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>quasars</subject><subject>active-galactic-nuclei</subject><subject>radial-velocity</subject><subject>line-intensities</subject><description>We investigate broad absorption line (BAL) disappearance and emergence using a 470 BAL-quasar sample over &lt;=0.10-5.25 rest-frame years with at least three spectroscopic epochs for each quasar from the Sloan Digital Sky Survey. We identify 14 disappearing BALs over &lt;=1.73-4.62 rest-frame years and 18 emerging BALs over &lt;=1.46-3.66 rest-frame years associated with the CIV{lambda}{lambda}1548,1550 and/or SiIV{lambda}{lambda}1393,1402 doublets, and report on their variability behaviour. BAL quasars in our data set exhibit disappearing/emerging C IV BALs at a rate of 2.3^+0.9^_-0.7_ and 3.0^+1.0^_-0.8_ per cent, respectively, and the frequency for BAL to non-BAL quasar transitions is 1.7^+0.8^_-0.6_ per cent. We detect four re-emerging BALs over &lt;=3.88 rest-frame years on average and three re-disappearing BALs over &lt;=4.15 rest-frame years on average, the first reported cases of these types. We infer BAL lifetimes along the line of sight to be nominally &lt;=100-1000yr using disappearing CIV BALs in our sample. Interpretations of (re-)emerging and (re-)disappearing BALs reveal evidence that collectively supports both transverse-motion and ionization-change scenarios to explain BAL variations. We constrain a nominal CIV/SiIV BAL-outflow location of &lt;=100pc from the central source and a radial size of &gt;=1x10^-7^pc (0.02au) using the ionization-change scenario, and constrain a nominal outflow location of &lt;=0.5pc and a transverse size of ~0.01pc using the transverse-motion scenario. Our findings are consistent with previous work, and provide evidence in support of BALs tracing compact flow geometries with small filling factors.</description><source format="bibcode">2017MNRAS.469.3163M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/469/3163</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/J/MNRAS/405/2302">J/MNRAS/405/2302 : Improved redshifts for SDSS quasar spectra (Hewett+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/45">J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 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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>T2</name><description>indicates disappearing and emerging BALs properties in table2</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Name</name><description>BAL quasar name (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType><flag>primary</flag></column><column><name>PMF</name><description>Plate-MJD-Fiber number for the associated SDSS spectrum</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Vmin</name><description>Minimum BAL velocity (1)</description><unit>km/s</unit><ucd>phys.veloc;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Vmax</name><description>Maximum BAL velocity (1)</description><unit>km/s</unit><ucd>phys.veloc;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BI</name><description>Balnicity index</description><unit>km/s</unit><ucd>meta.code;spect.index</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>EW</name><description>Rest-frame equivalent width</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sp</name><description>Interactive spectrum from SDSS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position from Name (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from Name (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/MNRAS/469/3163/table2</name><description>Properties of BAL quasars with pristine disappearing and emerging BALs</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>Flag</name><description>[DE] Disappearing (D) or Emerging (E) BALs</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Name</name><description>BAL-quasar name (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>n_Name</name><description>[BW ] Note on Name (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>z</name><description>Emission-line redshift (Hewett &amp; Wild, 2010, Cat. 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