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相关论文: Star-Planet Interactions in X-rays

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Close-in, giant planets are expected to influence their host stars via tidal or magnetic interaction. But are these effects strong enough in suitable targets known so far to be observed with today's instrumentation? The upsilon And system,…

太阳与恒星天体物理 · 物理学 2015-05-20 K. Poppenhaeger , L. F. Lenz , A. Reiners , J. H. M. M. Schmitt , E. Shkolnik

Context. Signatures of chromospheric activity enhancement have been found for a dozen stars, pointing to a possible star-planet interaction. Nevertheless in the coronal activity regime, there is no conclusive observational evidence for such…

地球与行星天体物理 · 物理学 2011-05-06 B. L. Canto Martins , M. L. das Chagas , S. Alves , I. C. Leão , L. P. de Souza Neto , J. R. de Medeiros

Do extrasolar planets affect the activity of their host stars? Indications for chromospheric activity enhancement have been found for a handful of targets, but in the X-ray regime, conclusive observational evidence is still missing. We want…

太阳与恒星天体物理 · 物理学 2015-05-18 K. Poppenhaeger , J. Robrade , J. H. M. M. Schmitt

We investigate whether magnetic interaction between close-in giant planets and their host stars produce observable statistical enhancements in stellar coronal or chromospheric activity. New Chandra observations of 12 nearby (d<60 pc)…

高能天体物理现象 · 物理学 2015-06-23 Brendan P. Miller , Elena Gallo , Jason T. Wright , Elliott G. Pearson

Magnetic (or tidal) interactions between "hot Jupiters" and their host stars can potentially enhance chromospheric and coronal activity. An ideal testbed for investigating this effect is provided by the extreme WASP-18 system, which…

地球与行星天体物理 · 物理学 2015-06-05 Brendan P. Miller , Elena Gallo , Jason T. Wright , Andrea K. Dupree

The bright F8 V solar-type star upsilon Andromedae has recently been reported to have a system of three planets of Jovian masses. In order to investigate the orbital stability and mutual gravitational interactions among these extrasolar…

天体物理学 · 物理学 2009-10-31 Ing-Guey Jiang , Wing-Huen Ip

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 activity levels of stars are influenced by several stellar properties, such as stellar rotation, spectral type and the presence of stellar companions. In analogy to binaries, planetary companions are also thought to be able to cause…

太阳与恒星天体物理 · 物理学 2015-05-28 K. Poppenhaeger , J. H. M. M. Schmitt

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

The magnetic activity levels of planet host stars may differ from that of stars not known to host planets in several ways. Hot Jupiters may induce activity in their hosts through magnetic interactions, or through tidal interactions by…

太阳与恒星天体物理 · 物理学 2017-06-23 Jason T. Wright , Brendan P. Miller

Planets may have effects on their host stars by tidal or magnetic interaction. Such star-planet interactions are thought to enhance the activity level of the host star. However, stellar activity also affects the sensitivity of planet…

太阳与恒星天体物理 · 物理学 2013-03-05 K. Poppenhaeger , J. H. M. M. Schmitt

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

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

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

Most (~82%) of the over 4000 confirmed exoplanets known today orbit very close to their host stars, within 0.5 au. Planets at such small orbital distances can result in significant interactions with their host stars, which can induce…

地球与行星天体物理 · 物理学 2020-04-15 Gayathri Viswanath , Mayank Narang , P. Manoj , Blesson Mathew , Sreeja S Kartha

Several "hot Jupiter" host stars appear to exhibit enhanced chromospheric activity, coronal flaring, and starspot development synchronized to their planetary orbits. These effects have been attributed to tidal and/or magnetic interactions…

太阳与恒星天体物理 · 物理学 2019-02-14 Matthew Route

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 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

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

The magnetic activity of planet-hosting stars is an important factor to estimate the atmospheric stability of close-in exoplanets and the age of their host stars. It has long been speculated that close-in exoplanets can influence the…

太阳与恒星天体物理 · 物理学 2014-05-13 K. Poppenhaeger , S. J. Wolk
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