activity
20162024
most citedA planet within the debris disk around the pre-main-sequence star AU Microscopii

242 citations · 1.1k across the 22 of their papers we have counts for

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Showing astro-ph.SRShow all

13 papers · 1 filter

astro-ph.SR2021

Reconstructing the Extreme Ultraviolet Emission of Cool Dwarfs Using Differential Emission Measure Polynomials

Girish M. Duvvuri, J. Sebastian Pineda, Zachory K. Berta-Thompson +16

Characterizing the atmospheres of planets orbiting M dwarfs requires understanding the spectral energy distributions of M dwarfs over planetary lifetimes. Surveys like MUSCLES, HAZ…

astro-ph.SR2020

Estimating the Ultraviolet Emission of M dwarfs with Exoplanets from Ca II and H

Katherine Melbourne, Allison Youngblood, Kevin France +29

M dwarf stars are excellent candidates around which to search for exoplanets, including temperate, Earth-sized planets. To evaluate the photochemistry of the planetary atmosphere,…

astro-ph.SR202012 cited

TIC 278956474: Two close binaries in one young quadruple system, identified by \textit{TESS}

Pamela Rowden, Tamás Borkovits, Jon M. Jenkins +25

We have identified a quadruple system with two close eclipsing binaries in TESS data. The object is unresolved in Gaia and appears as a single source at parallax 1.08~0.01 mas…

astro-ph.SR202046 cited

Exploring the evolution of stellar rotation using Galactic kinematics

Ruth Angus, Angus Beane, Adrian M. Price-Whelan +9

The rotational evolution of cool dwarfs is poorly constrained after around 1-2 Gyr due to a lack of precise ages and rotation periods for old main-sequence stars. In this work we u…

astro-ph.SR202045 cited

Orbital Parameter Determination for Wide Stellar Binary Systems in the Age of Gaia

Logan A. Pearce, Adam L. Kraus, Trent J. Dupuy +4

The orbits of binary stars and planets, particularly eccentricities and inclinations, encode the angular momentum within these systems. Within stellar multiple systems, the magnitu…

astro-ph.SR20199 cited

Magnetic Inflation and Stellar Mass. V. Intensification and saturation of M dwarf absorption lines with Rossby number

Philip S. Muirhead, Mark J. Veyette, Elisabeth R. Newton +2

In young sun-like stars and field M dwarf stars, chromospheric and coronal magnetic activity indicators such as H, X-ray and radio emission are known to saturate with low Rossby…