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<ri:Resource created="2017-06-19T15:26:50Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>A survey for H{alpha} pulsar bow shocks</title><shortName>J/ApJ/784/154</shortName><identifier>ivo://CDS.VizieR/J/ApJ/784/154</identifier><altIdentifier>doi:10.26093/cds/vizier.17840154</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brownsberger S.</name></creator><creator><name>Romani R.W.</name></creator><date role="Updated">2017-10-16T08:55:53Z</date><date role="Created">2017-06-19T15:26:50Z</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>pulsars</subject><subject>gamma-ray-astronomy</subject><subject>visible-astronomy</subject><subject>h-alpha-photometry</subject><subject>stellar-distance</subject><subject>extinction</subject><description>We report on a survey for H{alpha} bow shock emission around nearby {gamma}-detected energetic pulsars. This survey adds three Balmer-dominated neutron star bow shocks to the six previously confirmed examples. In addition to the shock around Fermi pulsar PSR J1741-2054, we now report H{alpha} structures around two additional {gamma}-ray pulsars, PSR J2030+4415 and PSR J1509-5850. These are the first known examples of H{alpha} nebulae with pre-ionization halos. With new measurements, we show that a simple analytic model can account for the angular size and flux of the bow shocks' apices. The latter, in particular, provides a new pulsar probe and indicates large moments of inertia and smaller distances than previously assumed in several cases. In particular, we show that the re-measured PSR J0437-4715 shock flux implies I=(1.7+/-0.2)x10^45^/(f_H I_sin i)g cm^2^. We also derive a distance d~0.72 kpc for the {gamma}-ray only pulsar PSR J2030+4415 and revised distances for PSRs J1959+2048 (1.4 kpc) and J2555+6535 (~1 kpc), smaller than the conventional DM-estimated values. Finally, we report upper limits for 94 additional LAT pulsars. An estimate of the survey sensitivity indicates that for a warm neutral medium filling factor {phi}_WNM_~0.3 there should be a total of approximately nine H{alpha} bow shocks in our LAT-targeted survey; given that seven such objects are now known, a much larger {phi}_WNM_ seems problematic.</description><source format="bibcode">2014ApJ...784..154B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/784/154</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VII/189">VII/189 : Catalog of Pulsars (Taylor+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/273/411">J/MNRAS/273/411 : Multifrequency fluxes of 280 pulsars (Lorimer+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/405/2243">J/MNRAS/405/2243 : GMOS/WIYN spectroscopic catalogue (Trichas+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/424/2832">J/MNRAS/424/2832 : Pulsars in {gamma}-ray sources (Lee+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/17">J/ApJS/208/17 : 2nd Fermi LAT cat. of gamma-ray pulsars (2PC) (Abdo+, 2013)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/784/154</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/784/154</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/784/154</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/784/154</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/784/154</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/784/154</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Radio</waveband><waveband>Gamma-ray</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/784/154/table2</name><description>Pulsars with Flux Upper Limits</description><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>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>Pulsar name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Exp</name><description>W012 exposure time</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Tel</name><description>[GSW] Telescope/camera flag (1)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>fobs5</name><description>Measured H{alpha} flux limit at fixed scale (2)</description><unit>1e-05cm**-2.s**-1</unit><ucd>phot.flux.density;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>Distance</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Code</name><description>[DGKOP] Distance type code (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>AR</name><description>Estimated R band extinction</description><unit>mag</unit><ucd>phys.absorption;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pVel</name><description>Adopted perpendicular velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Spin</name><description>Spindown power (dE_34_/dt)</description><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>fmod5</name><description>Expected flux for the WNM model</description><unit>1e-05cm**-2.s**-1</unit><ucd>phot.flux.density;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_Ratio</name><description>[&gt;] Limit flag on Ratio</description><ucd>meta.code.error;arith.ratio</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Ratio</name><description>Ratio of observed limit to model flux at the model angular scales (4)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Thetamod</name><description>Model angular scale</description><unit>arcsec</unit><ucd>instr.scale;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_ThetaI</name><description>[&lt;&gt;] Limit flag on ThetaI</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>ThetaI</name><description>? 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