Differential rotation on both components of the pre‐main‐sequence binary system HD 155555

Differential rotation on both components of the pre‐main‐sequence binary system HD 155555

Source :

• Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2008-07-11.

Descripteurs français

• Pascal (Inist)
  • Age, Binaire spectroscopique, Champ magnétique, Convection, Couronne stellaire, Etoile magnétique, Etoile séquence principale, Force rotation, Intensité, Modèle, Polarisation circulaire, Rotation différentielle, Rotation solaire, Rotation stellaire, Suite spectrale, Série temporelle, Tache stellaire, Type spectral.

English descriptors

• KwdEn :
  • Age, Binary, Binary orbit, Binary system, Binary systems, Brightness maps, Cameron, Characteristic signature, Circular polarization, Collier, Collier cameron, Complete phase coverage, Convection, Convection zone, Convection zone depth, Convection zone depths, Convection zones, Convective, Convective envelope, Crosscorrelation technique, Data sets, Differential, Differential rotation, Differential rotation curves, Differential rotation measurement, Differential rotation measurements, Differential rotation parameters, Differential rotation rate, Differential rotation rates, Differential rotation strength, Donati, Donati collier cameron, Donati rees, Donati semel, Doppler, Doppler imaging, Doppler imaging process, Dots code, Dunstone, Eld, Equatorial rotation rate, Evolutionary models, Evolutionary stage, Fractional radius, G5iv k0iv, Higher level, Hussain, Image shear, Image shear technique, Imaging, Imaging code, Imaging process, Independent maps, Intensity, Intensity spectra, Internal rotation, Internal structure, Internal velocity, Journal compilation, Large convection zone depths, Last section, Latitude, Latitude strip, Lled circle, Magnetic features, Magnetic fields, Magnetic images, Magnetic maps, Magnetic regions, Magnetic stars, Magnetic structures, Main sequence stars, Many advantages, Maps show, Marks show, Maximum ratio, Middle panel, Mnras, Models, Original paper, Physical parameters, Primary side, Primary star, Primary stars, Probability contours, Radiative core, Results show, Rotation, Rotation parameters, Rotation rate, Rotation strength, Rotational period, Second data, Second epoch, Secondary side, Secondary star, Secondary stars, Sheared image technique, Single star, Single stars, Solar rotation, Solid line, Solid triangles, Spectral sequence, Spectral type, Spectroscopic binary stars, Spot features, Spot maps, Star, Starspots, Stellar, Stellar convection zone, Stellar coronae, Stellar latitude, Stellar rotation, Stellar rotations, Stellar surface, Stokes, Strassmeier rice, Surface brightness distribution, Surface maps, Surface rotation parameters, Surface rotation properties, Synchronous rotation, Synchronously, Tidal, Tidal forces, Time series, Upper plot, Variable star, Vertical line.
• Teeft :
  • Binary, Binary orbit, Binary system, Binary systems, Brightness maps, Cameron, Characteristic signature, Collier, Collier cameron, Complete phase coverage, Convection, Convection zone, Convection zone depth, Convection zone depths, Convection zones, Convective, Convective envelope, Crosscorrelation technique, Data sets, Differential, Differential rotation, Differential rotation curves, Differential rotation measurement, Differential rotation measurements, Differential rotation parameters, Differential rotation rate, Differential rotation rates, Differential rotation strength, Donati, Donati collier cameron, Donati rees, Donati semel, Doppler, Doppler imaging, Doppler imaging process, Dots code, Dunstone, Eld, Equatorial rotation rate, Evolutionary models, Evolutionary stage, Fractional radius, G5iv k0iv, Higher level, Hussain, Image shear, Image shear technique, Imaging, Imaging code, Imaging process, Independent maps, Intensity spectra, Internal rotation, Internal structure, Internal velocity, Journal compilation, Large convection zone depths, Last section, Latitude, Latitude strip, Lled circle, Magnetic features, Magnetic images, Magnetic maps, Magnetic regions, Magnetic structures, Many advantages, Maps show, Marks show, Maximum ratio, Middle panel, Mnras, Original paper, Physical parameters, Primary side, Primary star, Primary stars, Probability contours, Radiative core, Results show, Rotation, Rotation parameters, Rotation rate, Rotational period, Second data, Second epoch, Secondary side, Secondary star, Secondary stars, Sheared image technique, Single star, Single stars, Solid line, Solid triangles, Spot features, Spot maps, Star, Stellar, Stellar convection zone, Stellar latitude, Stellar rotations, Stellar surface, Stokes, Strassmeier rice, Surface brightness distribution, Surface maps, Surface rotation parameters, Surface rotation properties, Synchronous rotation, Synchronously, Tidal, Tidal forces, Upper plot, Variable star, Vertical line.

Abstract

• https://api.istex.fr/document/FB9C57222BA64A0053C97EB7FEA46A15539C4593/fulltext/pdf
• https://api.istex.fr/document/E3541683166F62373048A99B00A2B86ABBB93161/fulltext/pdf

Affiliations:

• Allemagne, Australie, France, Royaume-Uni
• Midi-Pyrénées, Occitanie (région administrative)
• Toulouse

Links toward previous steps (curation, corpus...)

• to stream Istex, to step Corpus: 002F49
• to stream Istex, to step Curation: 002F49
• to stream Istex, to step Checkpoint: 001216
• to stream Istex, to step Corpus: 002A71
• to stream Istex, to step Curation: 002A71
• to stream Istex, to step Checkpoint: 001059
• to stream Main, to step Merge: 009110
• to stream PascalFrancis, to step Corpus: 003419
• to stream PascalFrancis, to step Curation: 002C30
• to stream PascalFrancis, to step Checkpoint: 003306
• to stream Main, to step Merge: 009720
• to stream Main, to step Curation: 008849

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