J/MNRAS/403/1368ivo://CDS.VizieR/J/MNRAS/403/1368doi:10.26093/cds/vizier.74031368CDSGonzalez G.Carlson M.K.Tobin R.W.2024-07-10T20:17:27Z2010-11-28T06:33:06ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetschemical-abundancesWe determine Li abundances and vsini values from new spectra of 53 stars with Doppler-detected planets not included in our previous papers in this series. We also examine two sets of stars without detected planets, which together serve as our comparison sample. Using the method of comparison of Li abundances and vsini values between two sets of stars we introduced in Gonzalez, we confirm that these two quantities are smaller among stars with planets (SWPs) compared to stars without detected planets near the solar temperature. The transition from low to high Li abundance among SWPs occurs near 5850K, a revision of about 50K from our previous determination. The transition from low to high vsini occurs near 6000K, but this temperature is not as well constrained.2010MNRAS.403.1368Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/403/1368CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/420/183 : Solar neighborhood spectroscopic survey (Allende Prieto+ 2004)J/MNRAS/378/1141 : Chemical abundances in 31 stars with planet (Gonzalez+ 2007)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/403/1368https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/403/1368http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/403/1368https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/403/1368https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/403/1368http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/403/1368GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/403/1368/stars (Parameters determined from our spectroscopic analyses of stars with planets: 53 new stars and re-analyses of stars in previous papers)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/403/1368/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/403/1368/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/403/1368/stars?GETtext/xml+votable180.050000true9.840858921.25047250.005555555555555556Cone search capability for table J/MNRAS/403/1368/table3 (Parameters determined for the comparison stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/403/1368/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/403/1368/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/403/1368/table3?GETtext/xml+votable180.050000true12.276213357.81518720.0055555555555555566/431 748 871 1341 1597 2110 2317 2416 2472 2476 3020 3102 3118 3876 3932 4136 4429 4528 4854 5067 5304 5522 5718 5836 6066 6760 6791 6821 7238 7240 7746 7763 8476 8614 8790 8843 8845 9179 9327 9443 9459 9476 9492 9553 9662 10225 10334 10375 10899 11087 11290 11326 12146 12465 12899 12983 14412 14416 14419 14434 16627 16652 17496 17730 19585 19904 19912 20072 20746 21003 21177 21838 21906 21956 22252 22300 22590 23123 23190 23201 23230 23646 23681 24019 24151 24178 24924 25939 26183 26242 26440 26521 26575 26963 26975 27088 27164 27616 27750 27975 28605 28882 29291 29513 29541 29598 30526 30837 30878 30943 30965 31029 31130 31374 31478 31768 31860 32035 32561 32575 35442 35532 35948 35954 36446 36506 36664 36697 39257 39364 39646 39926 40442 40692 42760 42887 43813 43911 44243 44398 46800 46967 48545https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/403/1368?format=asciiOpticaldefaultJ/MNRAS/403/1368/starsParameters determined from our spectroscopic analyses of stars with planets: 53 new stars and re-analyses of stars in previous papersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRSimbad column added by the CDSmeta.notecharHD? HD numbermeta.id;meta.mainintnullablem_HD[A] Multiplicity index on HDmeta.code.multipcharn_HD[ab] Different spectra for HD 170469 (2)meta.notecharHIP? HIP number (Cat. I/311)meta.idintnullableTeffEffective temperatureKphys.temperature.effectiveinte_Teffrms uncertainty on TeffKstat.error;phys.temperature.effectiveintloggSurface gravitylog(cm.s**-2)phys.gravityfloate_loggrms uncertainty on logglog(cm.s**-2)stat.errorfloatxiMicroturbulence velocitykm/sphys.veloc.microTurbfloate_xirms uncertainty on xikm/sstat.errorfloat[Fe/H]Metallicitylog(Sun)phys.abund.Zfloate_[Fe/H]rms uncertainty on [Fe/H]log(Sun)stat.error;phys.abund.Fefloatl_epsLiLimit flag on epsLimeta.code.errorcharepsLiLithium abundance (log scale, {epsilon}(H)=12)phys.abundfloate_epsLirms uncertainty on epsListat.errorfloatl_vsiniLimit flag on vsinimeta.code.error;phys.veloc.rotatcharvsiniRotational velocitykm/sphys.veloc.rotatfloate_vsinirms uncertainty on vsinikm/sstat.error;phys.veloc.rotatfloatMass? Mass derived from stellar isochronessolMassphys.massfloatnullablee_Mass? rms uncertainty on MasssolMassstat.error;phys.massfloatnullablelogg2? Gravity surface derived from stellar isochroneslog(cm.s**-2)phys.gravityfloatnullablee_logg2? rms uncertainty on logg2log(cm.s**-2)stat.errorfloatnullableAge? Age derived from stellar isochronesGyrtime.agefloatnullablee_Age? rms uncertainty on AgeGyrstat.error;time.agefloatnullableSampleSample for comparison stars (1)src.sampleSimbadNameSimbad column added by the CDSmeta.idchar_RAPosition from Simbad (right ascension part)degpos.eq.ra;meta.main_DEPosition from Simbad (declination part)degpos.eq.dec;meta.mainJ/MNRAS/403/1368/table3Parameters determined for the comparison starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHD? HD numbermeta.id;meta.mainintnullablem_HD[A] Multiplicity index on HDmeta.code.multipcharn_HD[ab] Different spectra for HD 170469 (2)meta.notecharHIP? HIP number (Cat. I/311)meta.idintnullableTeffEffective temperatureKphys.temperature.effectiveinte_Teffrms uncertainty on TeffKstat.error;phys.temperature.effectiveintloggSurface gravitylog(cm.s**-2)phys.gravityfloate_loggrms uncertainty on logglog(cm.s**-2)stat.errorfloatxiMicroturbulence velocitykm/sphys.veloc.microTurbfloate_xirms uncertainty on xikm/sstat.errorfloat[Fe/H]Metallicitylog(Sun)phys.abund.Zfloate_[Fe/H]rms uncertainty on [Fe/H]log(Sun)stat.error;phys.abund.Fefloatl_epsLiLimit flag on epsLimeta.code.errorcharepsLiLithium abundance (log scale, {epsilon}(H)=12)phys.abundfloate_epsLirms uncertainty on epsListat.errorfloatl_vsiniLimit flag on vsinimeta.code.error;phys.veloc.rotatcharvsiniRotational velocitykm/sphys.veloc.rotatfloate_vsinirms uncertainty on vsinikm/sstat.error;phys.veloc.rotatfloatMass? Mass derived from stellar isochronessolMassphys.massfloatnullablee_Mass? rms uncertainty on MasssolMassstat.error;phys.massfloatnullablelogg2? Gravity surface derived from stellar isochroneslog(cm.s**-2)phys.gravityfloatnullablee_logg2? rms uncertainty on logg2log(cm.s**-2)stat.errorfloatnullableAge? Age derived from stellar isochronesGyrtime.agefloatnullablee_Age? rms uncertainty on AgeGyrstat.error;time.agefloatnullableSampleSample for comparison stars (1)src.sampleSimbadNameSimbad column added by the CDSmeta.idchar_RAPosition from Simbad *vizSimbad (right ascension part)degpos.eq.ra;meta.main_DEPosition from Simbad *vizSimbad (declination part)degpos.eq.dec;meta.main