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<ri:Resource created="2018-08-08T14:16:29Z" 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>IR properties of stellar bowshock nebulae</title><shortName>J/AJ/154/201</shortName><identifier>ivo://CDS.VizieR/J/AJ/154/201</identifier><altIdentifier>doi:10.26093/cds/vizier.51540201</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kobulnicky H.A.</name></creator><creator><name>Schurhammer D.P.</name></creator><creator><name>Baldwin D.J.</name></creator><creator><name>Chick W.T.</name></creator><creator><name>Dixon D.M.,Lee D.</name></creator><creator><name>Povich M.S.</name></creator><date role="Updated">2018-08-27T08:05:45Z</date><date role="Created">2018-08-08T14:16:29Z</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>nebulae</subject><subject>galaxy-classification-systems</subject><subject>ob-stars</subject><subject>infrared-photometry</subject><subject>stellar-spectral-types</subject><subject>effective-temperature</subject><subject>stellar-radii</subject><subject>stellar-distance</subject><subject>galaxy-planes</subject><subject>milky-way-galaxy</subject><description>Arcuate infrared nebulae are ubiquitous throughout the Galactic Plane and are candidates for partial shells, bubbles, or bowshocks produced by massive runaway stars. We tabulate infrared photometry for 709 such objects using images from the Spitzer Space Telescope, the Wide-field Infrared Explorer, and the Herschel Space Observatory (HSO). Of the 709 objects identified at 24 or 22 {mu}m, 422 are detected at the HSO 70 {mu}m bandpass. Of these, only 39 are detected at HSO 160 {mu}m. The 70 {mu}m peak surface brightnesses are 0.5-2.5 Jyr/arcmin^2^. Color temperatures calculated from the 24 to 70 {mu}m ratios range from 80 to 400 K. Color temperatures from 70 to 160 {mu}m ratios are systematically lower, 40-200 K. Both of these temperature are, on average, 75% higher than the nominal temperatures derived by assuming that dust is in steady-state radiative equilibrium. This may be evidence of stellar wind bowshocks sweeping up and heating-possibly fragmenting but not destroying-interstellar dust. Infrared luminosity correlates with standoff distance, R_0_, as predicted by published hydrodynamical models. Infrared spectral energy distributions are consistent with interstellar dust exposed to either single radiant energy density, U=10^3^-10^5^ (in more than half of the objects) or a range of radiant energy densities U_min_=25 to U_max_=10^3^-10^5^ times the mean interstellar value for the remainder. Hence, the central OB stars dominate the energetics, making these enticing laboratories for testing dust models in constrained radiation environments. The spectral energy densities are consistent with polycyclic aromatic hydrocarbon fractions q_PAH_~&lt;1% in most objects.</description><source format="bibcode">2017AJ....154..201K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/154/201</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/A+A/578/A45">J/A+A/578/A45 : E-BOSS. II. 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42155 42158 42159 42169 42170 42171 42172 42173 42207 42211 42216 42217 42220 42224 42225 42226 42228 42376 42378 42379 42387 42391 42392 42393 42396 42397 42400 42416 42421 42434 42435 42438 42439 42440 42441 42444 42445 42447 42450 42454 42457 42458 42460 42461 42462 42496 42498 42500 42501 42514 43013 43015 43017 43019 43020 43022 43025 43026 43035 43041 44360</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/154/201?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/154/201/table1</name><description>SST and HSO Photometry of Candidate Bowshock 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>ID</name><description>[1/709] Index number using the numeration of Kobulnicky et al. (2016, J/ApJS/227/18) (G1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Name given in Galactic coordinates (GLLL.llll+BB.bbbb)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000) (G2)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000) (G2)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Rad</name><description>[0/151] Angular radius of nebula</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Height</name><description>[1/242] Angular height of nebula</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_F3.6</name><description>[&lt;] Limit flag on F3.6</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F3.6</name><description>[0.001/8.707]? Spitzer IRAC flux at 3.6 microns</description><unit>Jy</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_F4.5</name><description>[&lt;] Limit flag on F4.5</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F4.5</name><description>[0.001/6.467]? Spitzer IRAC flux at 4.5 microns</description><unit>Jy</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_F5.8</name><description>[&lt;] Limit flag on F5.8</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F5.8</name><description>[0/23.422]? Spitzer IRAC flux at 5.8 microns</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_F8.0</name><description>[&lt;] Limit flag on F8.0</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F8.0</name><description>[0.001/18.191]? Spitzer IRAC flux at 8.0 microns</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F24</name><description>[0.021/1211.4]? Spitzer MIPS flux at 24 microns</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>l_F70</name><description>[&lt;] Limit flag on F70</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F70</name><description>[0.03/618]? Herschel PACS flux at 70 microns</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_F160</name><description>[&lt;] Limit flag on F160</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F160</name><description>[0.04/394]? Herschel PACS flux at 160 microns</description><unit>Jy</unit><ucd>phot.flux.density;em.mm.1500-3000GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>I70</name><description>[0.7/13357]? Peak Herschel PACS 70 microns surface brightness</description><unit>Jy.arcmin**-2</unit><ucd>phot.flux.density.sb;em.IR.60-100um;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>T24/70</name><description>[61/762]? Color temperature (1)</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>T70/160</name><description>[32/262]? Color temperature (G3)</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/AJ/154/201/table2</name><description>WISE and HSO Photometry of Candidate Bowshock Nebulae</description><column><name>l_F70</name><description>[&lt;] Limit flag on F70</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">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>ID</name><description>[13/691] Index number using the numeration of Kobulnicky et al. (2016, J/ApJS/227/18) (G1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Name given in Galactic coordinates (GLLL.llll+BB.bbbb)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000) (G2)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000) (G2)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Rad</name><description>[5/900]? Angular radius of nebula</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Height</name><description>[7/600]? Angular height of nebula</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>l_F3.4</name><description>[&lt;] Limit flag on F3.4</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F3.4</name><description>[0.001/6.25] WISE flux at 3.4 microns</description><unit>Jy</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_F4.6</name><description>[&lt;] Limit flag on F4.6</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F4.6</name><description>[0.001/7.995] WISE flux at 4.6 microns</description><unit>Jy</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_F12</name><description>[&lt;] Limit flag on F12</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F12</name><description>[0.001/51.32] WISE flux at 12 microns</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F22</name><description>[0.01/343.77] WISE flux at 22 microns</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F70</name><description>[0.09/482.2]? Herschel PACS flux at 70 microns</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_F160</name><description>[&lt;] Limit flag on F160</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F160</name><description>[0.15/134.8]? Herschel PACS flux at 160 microns</description><unit>Jy</unit><ucd>phot.flux.density;em.mm.1500-3000GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>I70</name><description>[3.5/52.7]? Peak Herschel PACS 70 microns surface brightness</description><unit>Jy.arcmin**-2</unit><ucd>phot.flux.density.sb;em.IR.60-100um;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>T22/70</name><description>[81/230]? Color temperature (1)</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>T70/160</name><description>[39/240]? Color temperature (G3)</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/AJ/154/201/table5</name><description>Derived Parameters for Stars with Known Characteristics</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">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>ID</name><description>[13/413] Index number using the numeration of Kobulnicky et al. (2016, J/ApJS/227/18)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name1</name><description>Common name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Name</name><description>Name given in Galactic coordinates (GLLL.llll+BB.bbbb)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>SpType</name><description>MK spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Teff</name><description>[17600/41500] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>R*</name><description>[5.4/30] Stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>[0.14/2.3] Distance</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist1</name><description>[3.7/193] Standoff distance of the nebula from the central star, in arsec</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist2</name><description>[0.02/1.24] Standoff distance of the nebula from the central star, in pc</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>U</name><description>[320/230000] Radiation density parameter (1)</description><ucd>phys.energy.density</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TSS</name><description>[43/128] Steady-state temperature of dust</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>T22/T70</name><description>[70/842] Color temperature derived from the 24/70 {mu}m ratio</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>T70/160</name><description>[69/240]? Color temperature derived from the 70/160 {mu}m ratio</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FIR</name><description>[1.4e-10/6.4e-08] Total flux of the nebula (in erg/s/cm^2^)</description><unit>mW.m**-2</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>L*/LIR</name><description>[8.4/5400] Ratio of stellar luminosity to nebular luminosity</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>