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20112022
most citedInteraction model for the gap equation

232 citations · 3.2k across the 47 of their papers we have counts for

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12 papers · 1 filter

astro-ph.SR2022★ 7 cited

X-ray Emission from the Exoplanet Hosting LTT 1445 Triple Star System

Alexander Brown, Cynthia S. Froning, Allison Youngblood +5

JWST will be able to observe the atmospheres of rocky planets transiting nearby M dwarfs. The M dwarf triple star system LTT 1445, at a distance of 6.86 pc, hosts some of the neare…

astro-ph.SR2022★ 10 cited

Testing Lyman alpha emission line reconstruction routines at multiple velocities in one system

David J. Wilson, Allison Youngblood, Odette Toloza +6

The 1215.67A HI Lyman alpha emission line dominates the ultraviolet flux of low mass stars, including the majority of known exoplanet hosts. Unfortunately, strong attenuation by th…

astro-ph.SR2021★ 10 cited

Discovery of a young pre-intermediate polar

David J. Wilson, Odette Toloza, John D. Landstreet +4

We present the discovery of a magnetic field on the white dwarf component in the detached post common envelope binary (PCEB) CC Cet. Magnetic white dwarfs in detached PCEBs are ext…

astro-ph.SR2021★ 14 cited

8.9-hr Rotation in the Partly Burnt Runaway Stellar Remnant LP 40-365 (GD 492)

J. J. Hermes, Odelia Putterman, Mark A. Hollands +5

We report the detection of 8.914-hr variability in both optical and ultraviolet light curves of LP 40-365 (also known as GD 492), the prototype for a class of partly burnt runaway…

astro-ph.SR2021★ 67 cited

The Mega-MUSCLES Spectral Energy Distribution Of TRAPPIST-1

David J. Wilson, Cynthia S. Froning, Girish M. Duvvuri +19

We present a 5A-100um Spectral Energy Distribution (SED) of the ultracool dwarf star TRAPPIST-1, obtained as part of the Mega-MUSCLES Treasury Survey. The SED combines ultraviolet…

astro-ph.SR2021★ 50 cited

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…