46 citations · 111 across the 23 of their papers we have counts for
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Open Clusters as Laboratories for Cool Star Evolution: Highlights from the Cool Stars 23 Splinter Session
Deepak Chahal, Beatrice Caccherano, Edward Gillen +16
Open clusters remain among the most powerful laboratories for calibrating how fundamental stellar properties such as rotation, magnetic activity, surface chemistry, and internal st…
Radial and Rotational Velocities of a Volume-Complete Sample of M Dwarfs with Masses 0.1-0.3 Msun within 15 parsecs
Jennifer G. Winters, Emily K. Pass, David Charbonneau +7
We present the results from a five-year campaign to gather multi-epoch, high-resolution spectra of a volume-complete sample of 413 M dwarfs with masses 10-30% that of the Sun that…
Radio Burst from a Stellar Coronal Mass Ejection
J. R. Callingham, C. Tasse, R. Keers +15
Coronal mass ejections (CMEs) are massive expulsions of magnetised plasma from a star, and are the largest contributors to space weather in the Solar System. CMEs are theorized to…
Metallicities from High-Resolution TRES Spectra with uberMS: Performance Benchmarks and Literature Comparison
Emily K. Pass, Phillip A. Cargile, Victoria DiTomasso +7
As the field of exoplanetary astronomy has matured, demand has grown for precise stellar abundances to probe subtle correlations between stellar compositions and planetary demograp…
The Mass Dependence of Hα Emission and Stellar Spindown for Fully Convective M Dwarfs
Emily K. Pass, David Charbonneau, David W. Latham +4
Fully convective M dwarfs typically remain rapidly rotating and magnetically active for billions of years, followed by an abrupt and mass-dependent transition to slow rotation and…
Active Stars in the Spectroscopic Survey of Mid-to-Late M Dwarfs Within 15pc
Emily K Pass, Jennifer G Winters, David Charbonneau +2
We present results from the volume-complete spectroscopic survey of 0.1-0.3M M dwarfs within 15pc. This work discusses the active sample without close binary companions, pr…
G 68-34: A Double-Lined M-Dwarf Eclipsing Binary in a Hierarchical Triple System
Emily K Pass, David Charbonneau
Using high-resolution spectra from the Tillinghast Reflector Echelle Spectrograph (TRES) and photometry from sector 56 of the Transiting Exoplanet Survey Satellite (TESS), we repor…
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…