Imagen de Portada

Detecting and characterising the magnetic field of exoplanets

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Strugarek, A., Berdyugina, S. V., Bourrier, V., Caballero, J. A., Chebly, J. J., Fares, R., Fludra, A., Fossati, L., Muñoz, A. García, Gkouvelis, L., Gourvès, C., Grenfell, J. L., Kavanagh, R. D., Kislyakova, K. G., Lamy, L., Lanza, A. F., Moutou, C., Nandy, D., Neiner, C., Oklopčić, A., Paul, A., Réville, V., Rodgers-Lee, D., Shkolnik, E. L., Turner, J. D., Vidotto, A. A., Yang, F., Zarka, P.
Formato:	Preprint
Publicado:	2025
Materias:	Instrumentation and Methods for Astrophysics Earth and Planetary Astrophysics Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

A predictive framework for realistic star planet radio emission in compact systems
por: Chebly, J. J., et al.
Publicado: (2025)

Sungrazer comets as analogs of star-planet magnetic interactions
por: Guité, L-S., et al.
Publicado: (2026)

Introduction to magnetic star-planet interactions
por: Strugarek, A., et al.
Publicado: (2025)

Searching for magnetic fields in featureless white dwarfs with the DIPOL-UF polarimeter at the Nordic Optical Telescope
por: Berdyugin, A., et al.
Publicado: (2024)

Rotational evolution of young-to-old stars with data-driven three-dimensional wind models
por: Evensberget, D., et al.
Publicado: (2024)

Non-transiting exoplanets as a means of understanding star-planet interactions in close-in systems
por: Gourvès, C., et al.
Publicado: (2025)

Study of the atmospheric effects of energetic particle precipitations on giant planets with HWO
por: Chaufray, J-Y., et al.
Publicado: (2025)

The Neptunian ridge as a natural outcome of high-eccentricity tidal migration
por: Castro-González, A., et al.
Publicado: (2026)

Signs of magnetic star-planet interactions in HD 118203. TESS detects stellar variability that matches the orbital period of a close-in eccentric Jupiter-sized companion
por: Castro-González, A., et al.
Publicado: (2024)

Looking into the Jet Cone of the Neutrino-Associated Very High Energy Blazar PKS 1424+240
por: Kovalev, Y. Y., et al.
Publicado: (2025)

Mapping the exo-Neptunian landscape. A ridge between the desert and savanna
por: Castro-González, A., et al.
Publicado: (2024)

Metal accretion scars may be common on magnetic, polluted white dwarfs
por: Bagnulo, S., et al.
Publicado: (2024)

Unveiling the Diversity of Type IIn Supernovae via Systematic Light Curve Modeling
por: Ransome, C. L., et al.
Publicado: (2024)

Investigating Circumstellar Atomic Radiation-driven Dynamics
por: Lehtmets, A., et al.
Publicado: (2025)

Fundamental effective temperature measurements for eclipsing binary stars -- VI. Improved methodology and application to the circumbinary planet host star BEBOP-3
por: Maxted, P. F. L., et al.
Publicado: (2025)

Dynamical Masses for 23 Pre-Main Sequence Stars in Upper Scorpius: A Critical Test of Stellar Evolutionary Models
por: Towner, A. P. M., et al.
Publicado: (2025)

High-resolution Ultraviolet-to-nearinfrared Characterization of Exoplanet Atmospheres
por: Cubillos, Patricio E., et al.
Publicado: (2025)

JWST: Deuterated PAHs, PAH-nitriles, and PAH Overtone and Combination Bands I: Program Description and First Look
por: Boersma, C., et al.
Publicado: (2023)

Confirmation of SRGt 062340.2-265751 as a nova-like cataclysmic variable with a possible magnetic nature
por: Cúneo, V. A., et al.
Publicado: (2025)

Ageing and dynamics of the tailed radio galaxies in Abell 2142
por: Bruno, L., et al.
Publicado: (2024)

The Gaia Ultracool Dwarf Sample -- IV. GTC/OSIRIS optical spectra of Gaia late-M and L dwarfs
por: Cooper, W. J., et al.
Publicado: (2024)

The impact of medium-width bands on the selection, and subsequent luminosity function measurements, of high-z galaxies
por: Adams, N. J., et al.
Publicado: (2025)

Six-yr SPIRou monitoring of the young planet-host dwarf AU Mic
por: Donati, J. -F., et al.
Publicado: (2025)

A BCool survey of stellar magnetic cycles
por: Bellotti, S., et al.
Publicado: (2024)

X-Shooting ULLYSES: Massive stars at low metallicity -- V. Effect of metallicity on surface abundances of O stars
por: Martins, F., et al.
Publicado: (2024)

Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA
por: Bisigello, L., et al.
Publicado: (2024)

Star-Planet Interactions: A Computational View
por: Vidotto, A. A.
Publicado: (2025)

Spectropolarimetric characterisation of exoplanet host stars in preparation of the Ariel mission. Magnetic environment of HD 63433
por: Bellotti, S., et al.
Publicado: (2024)

Eating planets makes you younger: The magnetic dynamo rejuvenation of GJ 504 by planetary engulfment
por: Bellotti, S., et al.
Publicado: (2026)

High-precision astrometry with VVV -- II. A near-infrared extension of Gaia into the Galactic plane
por: Griggio, M., et al.
Publicado: (2024)

Connecting radio emission to AGN wind properties with Broad Absorption Line Quasars
por: Petley, J. W., et al.
Publicado: (2022)

Novel insights into the Coma Cluster kinematics with DESI. I. Linking mass profile, orbital anisotropy, and galaxy populations
por: Pedratti, S., et al.
Publicado: (2026)

A circularly polarized low-frequency radio burst from the exoplanetary system HD 189733
por: Zhang, X., et al.
Publicado: (2025)

Radio Signatures of Star-Planet Interactions, Exoplanets, and Space Weather
por: Callingham, J. R., et al.
Publicado: (2024)

Mass loading of outflows from evolving Young Massive Clusters
por: Larkin, C. J. K., et al.
Publicado: (2025)

A magnetic field study of two fast-rotating, radio bright M dwarfs. StKM 1-1262 and V374 Peg
por: Bellotti, S., et al.
Publicado: (2025)

Multi-Dimensional MHD simulations of young Core-Collapse Supernova Remnants
por: Larkin, C. J. K., et al.
Publicado: (2026)

Analysing the highly irregular boundaries of solar pores
por: Duckenfield, T. J., et al.
Publicado: (2026)

A.C.I.D -- An Improved LSD Technique for Accurate Line Profile Retrieval
por: Dolan, L. S., et al.
Publicado: (2024)

On stellar hotspots due to star-planet magnetic interactions: How much power can actually be transmitted to the chromosphere?
por: Paul, Arghyadeep, et al.
Publicado: (2025)