Results 1 to 10 of about 79,370 (261)

Stellar magnetic activity – Star-Planet Interactions

open access: yesEPJ Web of Conferences, 2015
Stellar magnetic activity is an important factor in the formation and evolution of exoplanets. Magnetic phenomena like stellar flares, coronal mass ejections, and high-energy emission affect the exoplanetary atmosphere and its mass loss over time.
Poppenhaeger, K.
doaj   +3 more sources

Magnetic field, differential rotation and activity of the hot-Jupiter hosting star HD 179949 [PDF]

open access: yesAstronomy & Astrophysics, 2012
HD 179949 is an F8V star, orbited by a giant planet at ~8 R* every 3.092514 days. The system was reported to undergo episodes of stellar activity enhancement modulated by the orbital period, interpreted as caused by Star-Planet Interactions (SPIs).
A. C. Cameron   +46 more
core   +4 more sources

Planet-star interactions with precise transit timing

open access: yesAstronomy & Astrophysics, 2022
Context. Hot Jupiters on extremely short-period orbits are expected to be unstable due to tidal dissipation and spiral toward their host stars. That is because they transfer the angular momentum of the orbital motion through tidal dissipation into the stellar interior. Although the magnitude of this phenomenon is related to the physical properties of a
G. Maciejewski   +16 more
openaire   +5 more sources

The birth environment of planetary systems [PDF]

open access: yesRoyal Society Open Science, 2020
Star and planet formation are inextricably linked. In the earliest phases of the collapse of a protostar, a disc forms around the young star and such discs are observed for the first several million years of a star’s life.
Richard J. Parker
doaj   +1 more source

ROME. III. The Arecibo Search for Star–Planet Interactions at 5 GHz

open access: yesThe Astrophysical Journal, 2023
After nearly three decades of discovery, many exoplanetary systems have been studied and characterized in detail with one important exception: exoplanet magnetism.
Matthew Route, Alexander Wolszczan
doaj   +1 more source

GJ 357 d: Potentially Habitable World or Agent of Chaos?

open access: yesThe Astronomical Journal, 2023
Multiplanet systems provide important laboratories for exploring dynamical interactions within the range of known exoplanetary system architectures. One such system is GJ 357, consisting of a low-mass host star and three orbiting planets, the outermost ...
Stephen R. Kane, Tara Fetherolf
doaj   +1 more source

Interactions of exoplanets with their environment

open access: yesComptes Rendus. Physique, 2023
Exoplanets on close-in orbit are subject to intense interactions with their host star. They receive a strong irradiation from the star, trigger tides within their host, and stars and close-in planets can be magnetically connected.
Strugarek, Antoine
doaj   +1 more source

Planet-star interactions with precise transit timing. II. The radial-velocity tides and a tighter constraint on the orbital decay rate in the WASP-18 system

open access: yesActa Astronomica, 2020
From its discovery, the WASP-18 system with its massive transiting planet on a tight orbit was identified as a unique laboratory for studies on tidal planet-star interactions. In an analysis of Doppler data, which include five new measurements obtained with the HIRES/Keck-I instrument between 2012 and 2018, we show that the radial velocity signal of ...
Maciejewski, G.   +6 more
openaire   +4 more sources

Star-planet interactions: I. Stellar rotation and planetary orbits [PDF]

open access: yes, 2016
Context. As a star evolves, the planet orbits change with time due to tidal interactions, stellar mass losses, friction and gravitational drag forces, mass accretion and evaporation on/by the planet.
Bianda, Michele   +5 more
core   +3 more sources

Magnetic games between a planet and its host star: the key role of topology [PDF]

open access: yes, 2015
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 of the stellar
Brun, A. S.   +3 more
core   +2 more sources

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