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1
Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa422
Abstract: The search for exoplanetary radio emission has resulted in zero conclusive detections to date. Various explanations for this have been proposed, from the observed frequency range, telescope sensitivity, to beaming of the emission. In a…
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Keywords:
stellar wind;
wind host;
radio;
host ... See more keywords
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2
Published in 2023 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stad925
Abstract: F stars lie in the transition region between cool stars with dynamo generated fields and hot star fossil fields and offer an interesting window into the generation of magnetic fields in shallow convection zones. In…
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Keywords:
star;
mature;
magnetic field;
stellar wind ... See more keywords
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0
Published in 2017 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stx1543
Abstract: Winds of cool dwarfs are difficult to observe, with only a few M dwarfs presenting observationally-derived mass-loss rates (Mdot), which span several orders of magnitude. Close-in exoplanets are conveniently positioned in the inner regions of…
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Keywords:
stellar wind;
wind;
exoplanets probes;
host stars ... See more keywords
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1
Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty1198
Abstract: Mass and energy injection throughout the lifetime of a star cluster contributes to the gas reservoir available for subsequent episodes of star formation and the feedback energy budget responsible for ejecting material from the cluster.…
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Keywords:
retention expulsion;
stellar wind;
star clusters;
retention ... See more keywords
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0
Published in 2017 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnrasl/slw206
Abstract: Stellar winds govern the angular momentum evolution of solar-like stars throughout their main-sequence lifetime. The efficiency of this process depends on the geometry of the star's magnetic field. There has been a rapid increase recently…
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Keywords:
stellar wind;
resolution;
angular momentum;
geometry ... See more keywords
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1
Published in 2019 at "Astronomy Reports"
DOI: 10.1134/s1063772919070096
Abstract: We show that the orbits of exoplanets of the "hot Jupiter" type, as a rule, are located close to the Alfven point of the stellar wind of the parent star. At this, many hot Jupiters…
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Keywords:
possible types;
types magnetospheres;
magnetic field;
hot jupiters ... See more keywords