593 citations · 8.7k across the 134 of their papers we have counts for
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Planets Around Low-Mass Stars (PALMS). IV. The Outer Architecture of M Dwarf Planetary Systems
Brendan P. Bowler, Michael C. Liu, Evgenya L. Shkolnik +1
We present results from a high-contrast adaptive optics imaging search for giant planets and brown dwarfs (>1 MJup) around 122 newly identified nearby (<40 pc) young M dwarfs. Half…
Herschel/PACS view of disks around low-mass stars and brown dwarfs in the TW Hya association
Yao Liu, Gregory J. Herczeg, Munan Gong +6
We conducted Herschel/PACS observations of five very low-mass stars or brown dwarfs located in the TW Hya association with the goal of characterizing the properties of disks in the…
Predicting Lyman-alpha and Mg II Fluxes from K and M Dwarfs Using GALEX Ultraviolet Photometry
Evgenya L. Shkolnik, Kristina A. Rolph, Sarah Peacock +1
A star's UV emission can greatly affect the atmospheric chemistry and physical properties of closely orbiting planets with the potential for severe mass loss. In particular, the Ly…
HAZMAT I: The Evolution of Far-UV and Near-UV Emission from Early M Stars
Evgenya L. Shkolnik, Travis S. Barman
The spectral energy distribution, variability and evolution of the high-energy radiation from an M dwarf planet host is crucial in understanding the planet's atmospheric evolution…
Secular orbital evolution of planetary systems and the dearth of close-in planets around fast rotators
A. F. Lanza, E. L. Shkolnik
Recent analyses of Kepler space telescope data reveal that transiting planets with orbital periods shorter than about 2-3 days are generally observed around late-type stars with ro…
A Stellar Census of the Tucana-Horologium Moving Group
Adam L. Kraus, Evgenya L. Shkolnik, Katelyn N. Allers +1
We report the selection and spectroscopic confirmation of 129 new late-type (K3-M6) members of the Tuc-Hor moving group, a nearby (~40 pc), young (~40 Myr) population of comoving s…