constraints on the radial differential rotation of six sun-like stars martin bo nielsen laurent...
TRANSCRIPT
Constraints on the radial Constraints on the radial differential rotation of six differential rotation of six
Sun-like starsSun-like stars
Martin Bo NielsenMartin Bo NielsenLaurent Gizon, Hannah Schunker Laurent Gizon, Hannah Schunker
and Jesper Schouand Jesper SchouInstitute for Astrophysics GöttingenInstitute for Astrophysics Göttingen
Max Planck Institute for Solar System ResearchMax Planck Institute for Solar System Research
Dec. 5Dec. 5thth 2014 2014Plato 2.0 Science Conference, Taormina, Plato 2.0 Science Conference, Taormina,
ItalyItaly
Internal rotation, why do we Internal rotation, why do we care?care? Stellar dynamosStellar dynamos
Differential rotationDifferential rotation Shear layer regenerates Shear layer regenerates
magnetic fieldmagnetic field
GyrochronologyGyrochronology Stellar windStellar wind Internal angular Internal angular
momentum?momentum?
Stellar modelsStellar models Structure and evolutionStructure and evolution
Schou et al. (1998)
Martin Nielsen, Plato 2.0
Martin Nielsen, Plato 2.0
AsteroseismologyAsteroseismology
CoRoT – HD52265 Kepler – HAT-P-7
Gizon et al. 2013 Lund et al. 2014
Martin Nielsen, Plato 2.0
StarStar Teff [K]*Teff [K]* logg [cm/s/s]*logg [cm/s/s]* Spot rotation Spot rotation period [days]period [days]
KIC004914923 5808±92 4.28±0.21 2424
KIC005184732 5669±97 4.07±0.21 2121
KIC006106415 6050±70 4.40±0.08 --
KIC006116048 5991±124 4.09±0.21 1818
KIC006933899 5837±97 4.21±0.22 3232
KIC010963065 6097±130 4.00±0.21 1212
*Molenda-Żakowicz et al. 2013
Six Sun-like Kepler StarsSix Sun-like Kepler Stars
Martin Nielsen, Plato 2.0
PeakbaggingPeakbagging
l=2m = 0,±1,±2
l=1m = 0,±1
l=0
Martin Nielsen, Plato 2.0
Splitting and inclinationSplitting and inclination
Nielsen et al. (2014)
Martin Nielsen, Plato 2.0
Spot rotation vs. asteroseismologySpot rotation vs. asteroseismology
Davies et al. in prep.
Martin Nielsen, Plato 2.0
SummarySummary Constrained radial differential rotation for six Sun-Constrained radial differential rotation for six Sun-
like stars.like stars.
Appears very consistent with comparison to solar Appears very consistent with comparison to solar data.data.
Rotation periods measured by asteroseismology Rotation periods measured by asteroseismology and starspots are consistent.and starspots are consistent.
Possible improvements: Possible improvements: Fitting ensembles of PLATO starsFitting ensembles of PLATO stars Accurate treatment of mode widthsAccurate treatment of mode widths Fit using specific profile (e.g. step function) Fit using specific profile (e.g. step function)
Thank you