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相关论文: Classification of magnetized star--planet interact…

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There are several physical processes that mediate the interaction between an exoplanet and its host star, with the four main ones being due to magnetic, particle (stellar outflow), radiative and tidal interactions. These interactions can be…

地球与行星天体物理 · 物理学 2025-06-03 A. A. Vidotto

Planets interact with their host stars through gravity, radiation and magnetic fields, and for those giant planets that orbit their stars within ~10 stellar radii (~0.1 AU for a sun-like star), star-planet interactions (SPI) are observable…

太阳与恒星天体物理 · 物理学 2024-12-13 Evgenya L. Shkolnik , Joe Llama

Magnetic interactions between a star and a close-in planet are postulated to be a source of enhanced emissions and to play a role in the secular evolution of the orbital system. Close-in planets generally orbit in the sub-alfv\'enic region…

地球与行星天体物理 · 物理学 2015-12-23 A. Strugarek , A. S. Brun , S. P. Matt , V. Réville

The interaction between planets and their host stars is governed by the forces of gravity, radiation, and magnetic fields. For planets orbiting their stars at distances of approximately 10 stellar radii or less, these effects are…

地球与行星天体物理 · 物理学 2025-02-20 A. Strugarek , E. Shkolnik

Stars and their exoplanets evolve together. Depending on the physical characteristics of these systems, such as age, orbital distance and activity of the host stars, certain types of star-exoplanet interactions can dominate during given…

太阳与恒星天体物理 · 物理学 2020-09-30 A. A. Vidotto

Planets in close-in orbit interact with the magnetized wind of their hosting star. This magnetic interaction was proposed to be a source for enhanced emissions in the chromosphere of the star, and to participate in setting the migration…

地球与行星天体物理 · 物理学 2016-12-21 A Strugarek

We present 2D magnetohydrodynamic simulations performed with the PLUTO code to model magnetized star-planet interactions. We study two simple scenarios of magnetized star-planet interactions: the unipolar and dipolar interactions. Despite…

太阳与恒星天体物理 · 物理学 2013-01-23 A. Strugarek , A. S. Brun , S. Matt

Magnetic interactions between a planet and its environment are known to lead to phenomena such as aurorae and shocks in the solar system. The large number of close-in exoplanets that were discovered triggered a renewed interest in magnetic…

地球与行星天体物理 · 物理学 2019-02-06 A. Strugarek

Evidence of magnetic interaction between late-type stars and close-in giant planets is provided by the observations of stellar hot spots rotating synchronously with the planets and showing an enhancement of chromospheric and X-ray fluxes.…

太阳与恒星天体物理 · 物理学 2015-05-13 A. F. Lanza

Close-in massive planets interact with their host stars through tidal and magnetic mechanisms. In this paper, we review circumstantial evidence for star-planet interaction as revealed by the photospheric magnetic activity in some of the…

太阳与恒星天体物理 · 物理学 2015-05-30 A. F. Lanza

Much effort has been invested in recent years, both observationally and theoretically, to understand the interacting processes taking place in planetary systems consisting of a hot Jupiter orbiting its star within 10 stellar radii. Several…

The outflowing magnetized wind from a host star shapes planetary and exoplanetary magnetospheres dictating the extent of its impact. We carry out three-dimensional (3D) compressible magnetohydrodynamic (MHD) simulations of the interactions…

地球与行星天体物理 · 物理学 2019-06-05 Srijan Bharati Das , Arnab Basak , Dibyendu Nandy , Bhargav Vaidya

The architecture of exoplanetary systems is often different from the solar system, with some exoplanets being in close orbits around their host stars and having orbital periods of only a few days. In analogy to interactions between stars in…

太阳与恒星天体物理 · 物理学 2019-05-15 Katja Poppenhaeger

Stars interact with their planets through gravitation, radiation, and magnetic fields. I shall focus on the interactions between late-type stars with an outer convection zone and close-in planets, i.e., with an orbital semimajor axis…

地球与行星天体物理 · 物理学 2014-08-27 A. F. Lanza

Recent observations suggest that stellar magnetic activity may be influenced by the presence of a close-by giant planet. Specifically, chromospheric hot spots rotating in phase with the planet orbital motion have been observed during some…

天体物理学 · 物理学 2009-11-13 A. F. Lanza

Forming planets around young, fast-rotating solar-like stars are exposed to an intense X-ray/extreme ultraviolet radiation field and strongly magnetized stellar winds, as a consequence of the high magnetic activity of these stars. Under…

地球与行星天体物理 · 物理学 2023-07-26 Ada Canet , Ana I. Gómez De Castro

The great majority of exoplanets discovered so far are orbiting cool, low-mass stars whose properties are relatively similar to the Sun. However, the stellar magnetism of these stars can be significantly different from the solar one, both…

太阳与恒星天体物理 · 物理学 2015-06-17 A. A. Vidotto

Magnetic interactions between a planet and its environment are known to lead to aurorae and shocks in the solar system. The large number of close-in exoplanets that have been discovered so far triggered a renewed interest in understanding…

太阳与恒星天体物理 · 物理学 2021-09-17 Antoine Strugarek

Late-type stars interact with their close-in planets through their coronal magnetic fields. We introduce a theory for the interaction between the stellar and planetary fields focussing on the processes that release magnetic energy in the…

地球与行星天体物理 · 物理学 2015-06-05 A. F. Lanza

Magnetic interactions between close-in planets and their host star can play an important role in the secular orbital evolution of the planets, as well as the rotational evolution of their host. As long as the planet orbits inside the…

地球与行星天体物理 · 物理学 2015-06-22 Antoine Strugarek , Allan Sacha Brun , Sean Patrick Matt , Victor Réville
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