355 citations · 3.8k across the 69 of their papers we have counts for
9 papers · 1 filter
Constraints on the Spindown of Fully-Convective M Dwarfs Using Wide Field Binaries
Emily K. Pass, David Charbonneau, Jonathan M. Irwin +1
M dwarfs remain active over longer timescales than their Sunlike counterparts, with potentially devastating implications for the atmospheres of their planets. However, the age at w…
Galactic Kinematics and Observed Flare Rates of a Volume-Complete Sample of Mid-to-Late M-dwarfs: Constraints on the History of the Stellar Radiation Environment of Planets Orbiting Low-mass Stars
Amber A. Medina, Jennifer G. Winters, Jonathan M. Irwin +1
We present a study of the relationship between galactic kinematics, flare rates, chromospheric activity, and rotation periods for a volume-complete, nearly all-sky sample of 219 si…
The POKEMON Speckle Survey of Nearby M Dwarfs. I. New Discoveries
Catherine A. Clark, Gerard T. van Belle, Elliott P. Horch +4
M dwarfs are favorable targets for exoplanet detection with current instrumentation, but stellar companions can induce false positives and inhibit planet characterization. Knowledg…
The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc
R. Luque, B. J. Fulton, M. Kunimoto +64
We report the discovery of a multi-planetary system transiting the M0 V dwarf HD 260655 (GJ 239, TOI-4599). The system consists of at least two transiting planets, namely HD 260655…
An Adaptive Optics Census of Companions to Northern Stars Within 25 pc with Robo-AO
Maissa Salama, Carl Ziegler, Christoph Baranec +8
In order to assess the multiplicity statistics of stars across spectral types and populations in a volume-limited sample, we censused nearby stars for companions with Robo-AO. We r…
Variability Timescales of H on Active Mid-to-Late M dwarfs
Amber A. Medina, David Charbonneau, Jennifer G. Winters +2
We present a study of the variation timescales of the chromospheric activity indicator H on a sample of 13 fully-convective, active mid-to-late M stars with masses between 0.1--…