J/MNRAS/411/L46ivo://CDS.VizieR/J/MNRAS/411/L46doi:10.26093/cds/vizier.74119046CDSVidotto A.A.Jardine M.Helling C.2024-07-13T20:14:44Z2011-10-17T18:02:34ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetsmagnetic-fieldsAn asymmetry between the ingress and egress times was observed in the near-UV light curve of the transit planet WASP-12b. Such asymmetry led us to suggest that the early ingress in the UV light curve of WASP-12b, compared to the optical observations, is caused by a shock around the planet, and that shocks should be a common feature in transiting systems. Here, we classify all the transiting systems known to date according to their potential for producing shocks that could cause observable light curve asymmetries.2011MNRAS.411L..46Vhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/411/L46CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/411/L46https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/411/L46http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/411/L46https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/411/L46https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/411/L46http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/411/L46GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/411/L46/table1 (*Transiting planetary systems known as of September 2010.)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/411/L46/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/411/L46/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/411/L46/table1?GETtext/xml+votable180.050000true97.636641729.67230280.0055555555555555566/790 876 1275 2335 2596 2711 3344 4990 5475 6017 6181 6381 6539 6638 7036 7208 8197 8825 9173 9355 9459 9482 9524 10654 10730 12424 12644 12853 12983 13439 13569 13680 13702 14772 14825-14826 14886 14914 14936 15040 15129 15143 15149 16947 17172 18766 20116 20339 22034 22040 22065 22078 22120 22208 22505 24409 25194 25950 28548 28821-28822 28864 30293 30450-30451 30466 31216 32727 32749 35210 36142 37246-37247 37329 37923 38452 42648 42936 43847 43960 44648 46421 46429 46437 47476https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/411/L46?format=asciidefaultJ/MNRAS/411/L46/table1*Transiting planetary systems known as of September 2010.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPlanetPlanet namemeta.id;meta.maincharMplPlanet mass, in M_{Jup}_ unit(1.898187x10+27kg)phys.massfloatRplPlanet radius, in R_{Jup}_ unitphys.size.radius;arith.ratiofloatPerOrbital perioddtime.periodfloatRorb? Orbital semi-major axisAUphys.size.smajAxisfloatnullableDist? Heliocentric distance to the systempcpos.distancefloatnullableSpTypeHost star MK spectral typemeta.idcharM*? Host star masssolMassphys.massfloatnullableR*? Host star RadiussolRadmeta.idfloatnullablevsini? Sky-projected stellar rotation velocitykm/sphys.veloc.rotatfloatnullablen_vsini[a] a: Gandolfi et al. (2010A&A...524A..55G)meta.notecharTmax? Maximum temperature required for shock formationMKphys.temperaturefloatnullablelognu? Local density around the planet for the confined coronalog(cm**-3)phys.densityfloatnullablelogns? Local density around the planet considering the coronal density scales with Omega*log(cm**-3)phys.densityfloatnullablerM(1)? Relative size of the planet magnetosphere for a planet with Bp=14G and a star with B*=1Gphys.size.radius;arith.ratiofloatnullablerM(100)? Relative size of the planet magnetosphere for a planet with Bp=14G and a star with B*=100Gphys.size.radius;arith.ratiofloatnullablef? Minimum planetary magnetic field relative to the stellar one (f=(Bp/B*)min) that is required to sustain a magnetosphere%phys.magFieldfloatnullableONameOther name of the planetmeta.idcharSimbadNameSimbad column added by the CDSmeta.idchar_RAPosition when known (the position of WASP-36 was not published) (right ascension part)degpos.eq.ra;meta.mainnullable_DEPosition when known (the position of WASP-36 was not published) (declination part)degpos.eq.dec;meta.mainnullable