most citedCoherent radio bursts from known M-dwarf planet host YZ Ceti

67 citations · 109 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2024

Binarity Enhances the Occurrence Rate of Radiation Belt Emissions in Ultracool Dwarfs

Melodie M. Kao, J. Sebastian Pineda

Despite a burgeoning set of ultracool dwarf (M7) radio detections, their radio emissions remain enigmatic. Open questions include the plasma source and acceleration mechanism…

astro-ph.SR2024

Impact of Electron Precipitation on Brown Dwarf Atmospheres and the Missing Auroral H Emission

J. Sebastian Pineda, Gregg Hallinan, Jean Michel Desert +1

Recent observations have demonstrated that very-low mass stars and brown dwarfs are capable of sustaining strong magnetic fields despite their cool and neutral atmospheres. These k…

astro-ph.SR2023

The High-Energy Spectrum of the Young Planet Host V1298 Tau

Girish M. Duvvuri, P. Wilson Cauley, Fernando Cruz Aguirre +4

V1298 Tau is a young pre-main sequence star hosting four known exoplanets that are prime targets for transmission spectroscopy with current-generation instruments. This work pieces…

astro-ph.SR20236 cited

Plausible association of distant late M dwarfs with low-frequency radio emission

A. J. Gloudemans, J. R. Callingham, K. J. Duncan +10

We present the serendipitous discovery of 8 distant ( 50 pc) late M dwarfs with plausible associated radio emission at 144 MHz. The M dwarf nature of our sources has been confir…

astro-ph.SR202318 cited

The winds of young Solar-type stars in the Pleiades, AB Doradus, Columba and Pictoris

Dag Evensberget, Stephen C. Marsden, Bradley D. Carter +6

Solar-type stars, which shed angular momentum via magnetised stellar winds, enter the main sequence with a wide range of rotational periods . This initially wide rang…

astro-ph.SR202367 cited

Coherent radio bursts from known M-dwarf planet host YZ Ceti

J. Sebastian Pineda, Jackie Villadsen

Observing magnetic star-planet interactions (SPI) offers promise for determining magnetic fields of exoplanets. Models of sub-Alfvénic SPI predict that terrestrial planets in close…