Results 11 to 20 of about 16,229 (284)

ON THE DETECTABILITY OF STAR-PLANET INTERACTION [PDF]

open access: yesThe Astrophysical Journal, 2012
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 features a massive (~10 times Jupiter) close-in (~1 day period) transiting planet orbiting a young F6 star. Optical and X-
Miller, Brendan P.   +3 more
openaire   +4 more sources

The corona of GJ 1151 in the context of star–planet interaction [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT The low-mass star GJ 1151 has been reported to display variable low-frequency radio emission, which has been interpreted as a signpost of coronal star–planet interactions with an unseen exoplanet. Here we report the first X-ray detection of GJ 1151’s corona based on the XMM–Newton data.
G Foster   +2 more
exaly   +4 more sources

The On/Off Nature of Star‐Planet Interactions [PDF]

open access: yesAstrophysical Journal, 2008
Evidence suggesting an observable magnetic interaction between a star and its hot Jupiter appears as a cyclic variation of stellar activity synchronized to the planet's orbit. In this study, we monitored the chromospheric activity of 7 stars with hot Jupiters using new high-resolution echelle spectra collected with ESPaDOnS over a few nights in 2005 ...
Evgenya L Shkolnik   +2 more
exaly   +4 more sources

III.9 Star-planet Interactions [PDF]

open access: yes, 2016
This book is dedicated to all the people interested in the CoRoT mission and the beautiful data that were delivered during its six year duration. Either amateurs, professional, young or senior researchers, they will find treasures not only at the time of this publication but also in the future twenty or thirty years. It presents the data in their final
Lanza, A. F., Ferraz-Mello, S.
openaire   +3 more sources

Planet-star interactions with precise transit timing

open access: yesAstronomy & Astrophysics
Aims. Tidal interactions shape the evolution of close-in giant planets and internal gravity-wave breaking offers an efficient pathway for dynamical-tide dissipation, although its population-wide impact remains poorly constrained.
Golonka J., Maciejewski G.
doaj   +2 more sources

Searching for Star-Planet interactions within the magnetosphere of HD 189733

open access: yes, 2010
HD 189733 is a K2 dwarf, orbited by a giant planet at 8.8 stellar radii. In order to study magnetospheric interactions between the star and the planet, we explore the large-scale magnetic field and activity of the host star. We collected spectra using the ESPaDOnS and the NARVAL spectropolarimeters, installed at the 3.6-m Canada-France-Hawaii telescope
Farès, R.   +9 more
openaire   +5 more sources

Star–planet interaction

open access: yesAstronomy & Astrophysics, 2022
Context. Electromagnetic star-planet interaction (SPI) describes the phenomenon of a planet coupling to its host star via electromagnetic forces. Alfvén waves can establish such a coupling by forming Alfvén wings. Star-planet interaction allows for phenomena that we do not otherwise know from the Solar System.
Fischer, C., Saur, J.
openaire   +3 more sources

Star-Planet Interactions

open access: yes, 2023
The exoplanet revolution that began three decades ago has drastically changed our knowledge of the extra-solar systems. Today, we face an extreme diversity and complexity of these systems that can only be understood through the intimate link that exists between the planets and their host stars.
Bigot, Lionel   +4 more
openaire   +3 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

Search for the Star-Planet Interaction [PDF]

open access: yesProceedings of the International Astronomical Union, 2011
AbstractWe analyse the chromospherical activity of stars with extrasolar planets and search for a possible correlation between the equivalent width of the core of the Ca II K line and orbital parameters of the planet. We found statistically significant evidence that the equivalent width of the Ca II K line reversal, which originates in the stellar ...
Tereza Krejčová   +2 more
openaire   +3 more sources

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