Moyano, F. D.; Eggenberger, P.; Mosser, B.; Spada, F.: Asteroseismology of evolved stars to constrain the internal transport of angular momentum. VI. Testing a parametric formulation for the azimuthal magneto-rotational instability. Astronomy and Astrophysics 673, S. A110 (2023)
Spada, F.; Demarque, P.; Kupka, F.: Stellar evolution models with entropy-calibrated mixing-length parameter: application to red giants. Monthly Notices of the Royal Astronomical Society 504 (3), S. 3128 - 3138 (2021)
Christensen-Dalsgaard, J.; Silva Aguirre, V.; Cassisi, S.; Miller Bertolami, M.; Serenelli, A.; Stello, D.; Weiss, A.; Angelou, G. C.; Jiang, C.; Lebreton, Y.et al.; Spada, F.; Bellinger, E. P.; Deheuvels, S.; Ouazzani, R. M.; Pietrinferni, A.; Mosumgaard, J. R.; Townsend, R. H. D.; Battich, T.; Bossini, D.; Constantino, T.; Eggenberger, P.; Hekker, S.; Mazumdar, A.; Miglio, A.; Nielsen, K. B.; Salaris, M.: The Aarhus red giants challenge: II. Stellar oscillations in the red giant branch phase. Astronomy and Astrophysics 635, A165 (2020)
Deheuvels, S.; Ballot, J.; Eggenberger, P.; Spada, F.; Noll, A.; den Hartogh, J. W.: Seismic evidence for near solid-body rotation in two Kepler subgiants and implications for angular momentum transport. Astronomy and Astrophysics 641, A117 (2020)
Gaulme, P.; Jackiewicz, J.; Spada, F.; Chojnowski, D.; Mosser, B.; McKeever, J.; Hedlund, A.; Vrard, M.; Benbakoura, M.; Damiani, C.: Active red giants: close binaries versus single rapid rotators. Astronomy and Astrophysics 639, A63 (2020)
Lehtinen, J.; Käpylä, M. J.; Olspert,, N.; Spada, F.: A Knee-Point in the Rotation-Activity Scaling of Late-type Stars with a Connection to Dynamo Transitions. (eingereicht)
Lehtinen, J.; Spada, F.; Käpylä, M. J.; Olspert, N.; Käpylä, P. J.: Common dynamo scaling in slowly rotating young and evolved stars. Nature astronomy 4, S. 658 - 662 (2020)
Silva Aguirre, V.; Christensen-Dalsgaard, J.; Cassisi, S.; Miller Bertolami, M.; Serenelli, A.; Stello, D.; Weiss, A.; Angelou, G. C.; Jiang, C.; Lebreton, Y.et al.; Spada, F.; Bellinger, E. P.; Deheuvels, S.; Ouazzani, R. M.; Pietrinferni, A.; Mosumgaard, J. R.; Townsend, R. H. D.; Battich, T.; Bossini, D.; Constantino, T.; Eggenberger, P.; Hekker, S.; Mazumdar, A.; Miglio, A.; Nielsen, K. B.; Salaris, M.: The Aarhus red giants challenge: I. Stellar structures in the red giant branch phase. Astronomy and Astrophysics 635, A164 (2020)
Spada, F.; Lanzafame, A. C.: Competing effect of wind braking and interior coupling in the rotational evolution of solar-like stars. Astronomy and Astrophysics 636, A76 (2020)
Eggenberger, P.; Deheuvels, S.; Miglio, A.; Ekström, S.; Georgy, C.; Meynet, G.; Lagarde, N.; Salmon, S.; Buldgen, G.; Montalbán, J.et al.; Spada, F.; Ballot, J.: Asteroseismology of evolved stars to constrain the internal transport of angular momentum: I. Efficiency of transport during the subgiant phase. Astronomy and Astrophysics 621, A66 (2019)
Lanzafame, A. C.; Distefano, E.; Barnes, S. A.; Spada, F.: Evidence of New Magnetic Transitions in Late-type Dwarfs from Gaia DR2. The Astrophysical Journal 877 (2), 157 (2019)
Spada, F.; Demarque, P.: Testing the entropy calibration of the radii of cool stars: models of α Centauri A and B. Monthly Notices of the Royal Astronomical Society 489 (4), S. 4712 - 4720 (2019)
Spada, F.; Arlt, R.; Küker, M.; Sofia, S.: Solar radius and luminosity variations induced by the internal dynamo magnetic fields. Astronomische Nachrichten 339 (7-8), S. 545 - 558 (2018)
Spada, F.; Demarque, P.; Basu, S.; Tanner, J. D.: Improved Calibration of the Radii of Cool Stars Based on 3D Simulations of Convection: Implications for the Solar Model. The Astrophysical Journal 869 (2), 135 (2018)
Erst eisige Kälte, dann Mitternachtssonne: Am Polarkreis bereitet das Team den Flug des ballongetragenen Sonnenobservatoriums vor – und hofft auf ein solares Feuerwerk.
Bewerbungsfrist 1 Oktober 2023. Promotionsprojekte in Planetenwissenschaften, Sonnenphysik, Astrophysik, Magnetfelder der Sonne, Helioseismologie, Asteroseismologie ...
In der mittleren Korona der Sonne entdeckt ein Forscherteam netzartige, dynamische Plasmastrukturen – und einen wichtigen Hinweis auf den Antrieb des Sonnenwindes.