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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

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

It has been proposed that magnetic activity could be enhanced due to interactions between close-in massive planets and their host stars. In this article, I present a brief overview of the connection between stellar magnetic activity and…

太阳与恒星天体物理 · 物理学 2017-11-08 A. A. Vidotto

Tidal interaction between an exoplanet and its host star is a possible pathway to transfer angular momentum between the planetary orbit and the stellar spin. In cases where the planetary orbital period is shorter than the stellar rotation…

太阳与恒星天体物理 · 物理学 2022-04-13 Nikoleta Ilic , Katja Poppenhaeger , S. Marzieh Hosseini

We present a spectropolarimetric snapshot survey of solar-type planet hosting stars. In addition to 14 planet-hosting stars observed as part of the BCool magnetic snapshot survey, we obtained magnetic observations of a further 19…

太阳与恒星天体物理 · 物理学 2016-11-24 M. W. Mengel , S. C. Marsden , B. D. Carter , J. Horner , R. King , R. Fares , S. V. Jeffers , P. Petit , A. A. Vidotto , J. Morin , the BCool Collaboration

Understanding the distribution of angular momentum during the formation of planetary systems is a key topic in astrophysics. Data from the $\textit{Kepler}$ and $\textit{Gaia}$ missions allow to investigate whether stellar rotation is…

地球与行星天体物理 · 物理学 2022-04-20 Yves Sibony , Ravit Helled , Robert Feldmann

The distribution of angular momentum of planets and their host stars provides important information on the formation and evolution of the planetary system. However, mysteries still remain, partly due to bias and uncertainty of the current…

地球与行星天体物理 · 物理学 2022-01-25 Jonathan H. Jiang , Remo Burn , Kristen A. Fahy , Xuan Ji , Patrick Eggenberger

The distribution of hot Jupiters, for which star-planet interactions can be significant, questions the evolution of exosystems. We aim to follow the orbital evolution of a planet along the rotational and structural evolution of the host…

Angular momentum is a key property regulating star formation and evolution. However, the physics driving the distribution of the stellar rotation rates of early-type main-sequence stars is as yet poorly understood. Using our catalog of…

太阳与恒星天体物理 · 物理学 2021-11-24 Weijia Sun , Xiao-Wei Duan , Licai Deng , Richard de Grijs

Both direct and indirect methods of exoplanet detection rely upon detailed knowledge of the potential host stars. Such stellar characterization allows for accurate extraction of planetary properties, as well as contributing to our overall…

地球与行星天体物理 · 物理学 2023-07-26 Emilie R. Simpson , Tara Fetherolf , Stephen R. Kane , Joshua Pepper , Teo Mocnik , Paul A. Dalba

The photospheric spot activity of some of the stars with transiting planets discovered by the CoRoT space experiment is reviewed. Their out-of-transit light modulations are fitted by a spot model previously tested with the total solar…

太阳与恒星天体物理 · 物理学 2015-05-20 A. F. Lanza

Starspots and their movements on stellar surfaces enable investigating the mechanisms of stellar magnetic activity. Information on the spot distribution and differential rotation provide important constraints for the behaviour of stellar…

太阳与恒星天体物理 · 物理学 2026-03-25 Mikko Tuomi , András Haris , Thomas Hackman

Rapid rotation enhances the dynamo operating in stars, and thus also introducessignificantly stronger magnetic activity than is seen in slower rotators. Many young cool stars still have the rapid, primordial rotation rates induced by the…

太阳与恒星天体物理 · 物理学 2015-06-03 H. Korhonen

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…

太阳与恒星天体物理 · 物理学 2017-03-08 K. Poppenhaeger

The rotation periods of the host stars of extrasolar planets have been assessed against those of the Mt. Wilson stars, open cluster stars, and evolutionary stellar models that include rotation. They appear to be normal, modulo certain…

天体物理学 · 物理学 2009-11-06 Sydney A. Barnes

The field of exoplanetary science is one of the most rapidly growing areas of astrophysical research. As more planets are discovered around other stars, new techniques have been developed that have allowed astronomers to begin to…

太阳与恒星天体物理 · 物理学 2015-03-20 B. A. Nicholson , M. W. Mengel , L. Brookshaw , A. A. Vidotto , B. D. Carter , S. C. Marsden , J. Soutter , I. A. Waite , J. Horner

We present rotation period measurements for subgiants observed by CoRoT. Interpreting the modulation of stellar light that is caused by star-spots on the time scale of the rotational period depends on knowing the fundamental stellar…

太阳与恒星天体物理 · 物理学 2012-10-30 J. -D. Jr. do Nascimento , J. S. da Costa , M. Castro

The Kepler mission revealed a plethora of stellar variability in the light curves of many stars, some associated with magnetic activity or stellar oscillations. In this work, we analyse the periodic signal in 162 intermediate-mass stars,…

Stellar activity is fundamental to stellar evolution and the formation and habitability of exoplanets. The interaction between convective motions and rotation in cool stars results in a dynamo process that drives magnetic surface activity.…

Roughly half of Solar-type planet hosts have stellar companions, so understanding how these binary companions affect the formation and evolution of planets is an important component to understanding planetary systems overall. Measuring the…

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