J/A+A/659/A71ivo://CDS.VizieR/J/A+A/659/A71doi:10.26093/cds/vizier.36590071CDSWillamo T.Lehtinen J.J.Hackman T.Kapyla M.J.Kochukhov O.,Jeffers S.V.Korhonen H.Marsden S.C.2022-09-06T14:05:07Z2022-03-09T17:46:57ZCDS support team

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

cds-question@unistra.frlate-type-starsmagnetic-fieldsThe magnetic activity of the Sun changes with the solar cycle. Similar cycles are found in other stars as well, but their details are not known to a similar degree. Characterising stellar magnetic cycles is important for the understanding of the stellar and solar dynamos that are driving the magnetic activity. We present spectropolarimetric observations of five young, solar-type stars and compare them to previous observations, with the aim to identify and characterise stellar equivalents of the solar cycle. We use Zeeman-Doppler imaging (ZDI) to map the surface magnetic field and brightness of our targets. The magnetic field is decomposed into spherical harmonic expansions, from which we report the strengths of the axisymmetric versus non-axisymmetric and poloidal versus toroidal components, and we compare them to the Rossby numbers of the stars. We present five new ZDI maps of young, solar-type stars from December 2017. Of special interest is the case of V1358 Ori, which had gone through a polarity reversal between our observations and earlier ones. A less evident polarity reversal might also have occurred in HD 35296. There is a preference for a more axisymmetric field, and possibly a more toroidal field, for the more active stars with lower Rossby number, but a larger sample should be studied to draw any strong conclusions from this. For most of the individual stars, the amounts of toroidal and poloidal field have stayed on levels similar to those in earlier observations. We find evidence for a magnetic polarity reversal having occurred in V1358 Ori. An interesting target for future observations is {chi}^1^ Ori, which may have a short magnetic cycle of a few years. The correlation between the brightness maps and the magnetic field is mostly poor, which could indicate the presence of small-scale magnetic features of different polarities that cancel one another out and are thus not resolved in our maps.2022A&A...659A..71Whttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/659/A71CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/659/A71https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/659/A71http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/659/A71https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/659/A71https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/659/A71http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/659/A71GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/659/A71/stars (List of studied stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/659/A71/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/659/A71/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/659/A71/stars?GETtext/xml+votable180.050000true5.7157917-12.20944440.0055555555555555566/17219 22146 24151 24160 34757https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/659/A71?format=asciidefaultJ/A+A/659/A71/starsList of studied starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameNamemeta.id;meta.maincharRAJ2000Simbad Hour of Right Ascension (J2000.0)pos.eq.ra;meta.mainDEJ2000Simbad Degree of Declination (J2000.0)pos.eq.dec;meta.mainFileNameName of the file with ZDI mapmeta.id;meta.filecharFileName2Name of the second file with ZDI mapmeta.id;meta.filecharSimbadSimbad column added by the CDSmeta.ref.urlcharJ/A+A/659/A71/becetZDI map of BE CetrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLatLatitudedegpos.framefloatLonLongitudedegpos.framefloatBradRadial magnetic fieldkGphys.magFielddoubleBmerMeridional magnetic fieldkGphys.magFielddoubleBaziAzimuthal magnetic fieldkGphys.magFielddoubleBrigNormalised brightnessphot.flux;em.opt;arith.ratiodoubleJ/A+A/659/A71/chi1oriZDI map of {chi}^1^ OrirecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLatLatitudedegpos.framefloatLonLongitudedegpos.framefloatBradRadial magnetic fieldkGphys.magFielddoubleBmerMeridional magnetic fieldkGphys.magFielddoubleBaziAzimuthal magnetic fieldkGphys.magFielddoubleBrigNormalised brightnessphot.flux;em.opt;arith.ratiodoubleJ/A+A/659/A71/hd29615ZDI map of HD 29615recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLatLatitudedegpos.framefloatLonLongitudedegpos.framefloatBradRadial magnetic fieldkGphys.magFielddoubleBmerMeridional magnetic fieldkGphys.magFielddoubleBaziAzimuthal magnetic fieldkGphys.magFielddoubleBrigNormalised brightnessphot.flux;em.opt;arith.ratiodoubleJ/A+A/659/A71/hd35296ZDI map of HD 35296recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLatLatitudedegpos.framefloatLonLongitudedegpos.framefloatBradRadial magnetic fieldkGphys.magFielddoubleBmerMeridional magnetic fieldkGphys.magFielddoubleBaziAzimuthal magnetic fieldkGphys.magFielddoubleBrigNormalised brightnessphot.flux;em.opt;arith.ratiodoubleJ/A+A/659/A71/v1358oriZDI map of V1358 OrirecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLatLatitudedegpos.framefloatLonLongitudedegpos.framefloatBradRadial magnetic fieldkGphys.magFielddoubleBmerMeridional magnetic fieldkGphys.magFielddoubleBaziAzimuthal magnetic fieldkGphys.magFielddoubleBrigNormalised brightnessphot.flux;em.opt;arith.ratiodoubleJ/A+A/659/A71/v1358or2ZDI map of V1358 Ori from September 2013BrigNormalised brightnessphot.flux;em.opt;arith.ratiodoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLatLatitudedegpos.framefloatLonLongitudedegpos.framefloatBradRadial magnetic fieldkGphys.magFielddoubleBmerMeridional magnetic fieldkGphys.magFielddoubleBaziAzimuthal magnetic fieldkGphys.magFielddouble