J/ApJ/776/67ivo://CDS.VizieR/J/ApJ/776/67doi:10.26093/cds/vizier.17760067CDSvan Saders J.L.Pinsonneault M.H.2019-03-26T09:39:55Z2015-06-11T08:21:38ZCDS support team

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

cds-question@unistra.fropen-star-clusterseffective-temperaturestellar-massesastronomical-modelsStellar rotation is a strong function of both mass and evolutionary state. Missions such as Kepler and CoRoT provide tens of thousands of rotation periods, drawn from stellar populations that contain objects at a range of masses, ages, and evolutionary states. Given a set of reasonable starting conditions and a prescription for angular momentum loss, we address the expected range of rotation periods for cool field stellar populations (~0.4-2.0M_{sun}_). We find that cool stars fall into three distinct regimes in rotation. Rapid rotators with surface periods less than 10 days are either young low-mass main sequence (MS) stars, or higher mass subgiants which leave the MS with high rotation rates. Intermediate rotators (10-40 days) can be either cool MS dwarfs, suitable for gyrochronology, or crossing subgiants at a range of masses. Gyrochronology relations must therefore be applied cautiously, since there is an abundant population of subgiant contaminants. The slowest rotators, at periods greater than 40 days, are lower mass subgiants undergoing envelope expansion. We identify additional diagnostic uses of rotation periods. There exists a period-age relation for subgiants distinct from the MS period-age relations. There is also a period-radius relation that can be used as a constraint on the stellar radius, particularly in the interesting case of planet host stars. The high-mass/low-mass break in the rotation distribution on the MS persists onto the subgiant branch, and has potential as a diagnostic of stellar mass. Finally, this set of theoretical predictions can be compared to extensive datasets to motivate improved modeling.2013ApJ...776...67Vhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/776/67CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/442/2081 : Praesepe members light curves (Kovacs+, 2014)J/A+A/560/A4 : Rotation periods of active Kepler stars (Reinhold+, 2013)J/A+A/557/L10 : Rotation periods of 12000 Kepler stars (Nielsen+, 2013)J/MNRAS/436/1883 : Properties of KOI host stars (Walkowicz+, 2013)J/MNRAS/432/1203 : Rotation periods of M-dwarf stars (McQuillan+, 2013)J/MNRAS/430/1433 : NGC 2264 members periods with CoRoT (Affer+, 2013)J/MNRAS/424/11 : Rotation of field stars from CoRoT data (Affer+, 2012)J/ApJS/199/30 : Temperature scale for KIC stars (Pinsonneault+, 2012)J/ApJ/746/16 : Modelling the convection zone (van Saders+, 2012)J/A+A/537/A120 : Rotational velocities of A-type stars. IV. (Zorec+, 2012)J/MNRAS/413/2218 : Stellar rotation in Hyades and Praesepe (Delorme+, 2011)J/AJ/142/112 : KIC photometric calibration (Brown+, 2011)J/ApJ/733/115 : Rotation periods and membership in M34 (Meibom+, 2011)J/A+A/523/A91 : CoRoT/Exoplanet fields with MATISSE (Gazzano+, 2010)J/MNRAS/408/475 : HATNet Pleiades Rotation Period Catalogue (Hartman+, 2010)J/ApJ/695/679 : Stellar rotation in M35 (Meibom+, 2009)J/ApJ/691/342 : griBVI photometry in M37 (Hartman+, 2009)J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008)J/ApJ/675/1233 : gri photometry in M37 (NGC 2099) (Hartman+, 2008)J/A+A/483/253 : BV photometry of NGC 2099 variables (Messina+, 2008)J/A+A/409/251 : Li abundances & velocities in F and G stars (Mallik+, 2003)J/A+A/397/147 : Activity-rotation relationship in stars (Pizzolato+ 2003)J/A+A/331/81 : Hyades membership (Perryman+ 1998)J/MNRAS/298/525 : Stellar evolution models for Z=0.0001 to 0.03 (Pols+ 1998)J/PASP/109/759 : Rotational Vel. of Intermediate-mass MS Stars (Wolff+ 1998)J/ApJS/99/135 : A-type stars rotation and spectral peculiarities (Abt+ 1995)J/PASP/96/707 : Hyades lower main sequence (Duncan+, 1984)http://www.univie.ac.at/webda/ : WEBDA database home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/776/67https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/776/67http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/776/67https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/776/67https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/776/67http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/776/67GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/776/67/table2 (Hyades & Praesepe rotation data)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/776/67/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/776/67/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/776/67/table2?GETtext/xml+votable180.050000true49.35994287.65581060.005555555555555556Cone search capability for table J/ApJ/776/67/table1 (M37 (NGC 2099) rotation data)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/776/67/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/776/67/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/776/67/table1?GETtext/xml+votable180.050000true87.82641666732.6755277780.0055555555555555565/5884 5886 6/75 309 320 322 333 336 337 339 340 342 348 349 351 353 375 1024 1032 1033 1035 1042 1058 1060 1075 4687 4696 4698 4699 4709 4720 4721 23335 23344 23383 23392 23396 23405 23416 23423 23438 23454 23463 23479 23489 23493 23497 23501 23502 23503 23514 23515 23518 23523 23525 23526 23527 23529 23532 23534 23535 23548 23658 24099 24104 24110 24137 24192 24194 24195 24201 24207 24218 24223 24315 24520 245223.322582951404819e-19 3.852589004194616e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/776/67?format=asciidefaultJ/ApJ/776/67/table2Hyades & Praesepe rotation dataSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeqWEBDA designation (1-187 for Hyades, 38-1133 for Praesepe) (1)meta.idintB-V[0.1/0.8] The (B-V) color index (2)magphot.color;em.opt.B;em.opt.VfloatMass[1/2.4] Mass (3)solMassphys.massfloatRad[0.9/3.1] Radius (3)solRadphys.size.radiusfloatvsini[1/245] Rotational velocity (2)km/sphys.veloc.rotatfloatPer[0.3/60.4] Rotation period (4)dtime.periodfloatCl[1/2] Cluster source (1=Hyades or 2=Praesepe)meta.codeint_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/ApJ/776/67/tracksRotational tracks for main-sequence and sub-giant branchs, metallicities [Fe/H]=0 or -0.2 (tables 3--6)tauConvective overturn timescale {tau}_c_stime.scaledoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[Fe/H]log(Sun)phys.abund.FefloatnullableEvmeta.id;stat.fitcharTeff[5000/7000] Effective temperature, step of 50KKphys.temperature.effectiveintlog(g)[3.5/4.7] Log of the surface gravity, step 0.005log(cm.s**-2)phys.gravityfloatMass[0.7/2] MasssolMassphys.massfloatlogL[-0.6/1.6] Log of the luminositylog(solLum)phys.luminosityfloatTeffZ[4865/10007] zero-age main sequence (ZAMS) derived effective temperatureKphys.temperature.effective;meta.mainintPfast[0.2/265] Fast launch model predicted rotation perioddtime.period;meta.modelleddoublePslow[2.4/267] Slow launch model predicted rotation perioddtime.period;meta.modelleddoubleItotMoment of inertiag.cm**2stat.variancedoubleJ/ApJ/776/67/table1M37 (NGC 2099) rotation datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[2/572] Star designation (1)meta.idintIDIdentification number in Hartman et al. 2009, J/ApJ/691/342 (<Cl* NGC 2099 HGH VNNNN> in Simbad)meta.id;meta.mainintVmag[15.7/22.9] V band magnitudemagphot.mag;em.opt.VfloatB-V[0.7/2] The (B-V) color indexmagphot.color;em.opt.B;em.opt.VfloatMass[0.3/1.3] Mass (2)solMassphys.massfloatPer[0.4/19.7] Rotation period (3)dtime.periodfloatSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPositions from Hartman et al. 2009, J/ApJ/691/342 (right ascension part)degpos.eq.ra;meta.main_DEPositions from Hartman et al. 2009, J/ApJ/691/342 (declination part)degpos.eq.dec;meta.main