activity
20082022
most citedPlacing the spotted T Tauri star LkCa 4 on an HR diagram

138 citations · 657 across the 24 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.SR201928 cited

The Mean Magnetic Field Strength of CI Tau

Kimberly R. Sokal, Christopher M. Johns-Krull, Gregory N. Mace +4

We present a blind comparison of two methods to measure the mean surface magnetic field strength of the classical T Tauri star CI Tau based on Zeeman broadening of sensitive spectr…

astro-ph.SR201919 cited

Chemical Abundances Of Open Clusters From High-Resolution Infrared Spectra. II. NGC 752

G. Böcek Topcu, M. Afsar, C. Sneden +9

We present a detailed near-infrared chemical abundance analysis of 10 red giant members of the Galactic open cluster NGC 752. High-resolution (R45000) near-infrared spectra…

astro-ph.SR2019

Compact Disks in a High Resolution ALMA Survey of Dust Structures in the Taurus Molecular Cloud

Feng Long, Gregory J. Herczeg, Daniel Harsono +24

We present a high-resolution (, au, mean sensitivity of Jy~beam at 225 GHz) snapshot survey of 32 protoplanetary disks around young stars with spe…

astro-ph.SR20191 cited

Radial Velocities of Low-mass Candidate TWA Members

Benjamin Kidder, Gregory Mace, Kimberly Sokal +2

Nearby young moving groups provide unique samples of similar age stars for testing the evolution of physical properties. Incomplete and/or incorrect group membership classification…

astro-ph.EP201935 cited

CO Detected in CI Tau b: Hot Start Implied by Planet Mass and M

Laura Flagg, Christopher M. Johns-Krull, Larissa Nofi +5

We acquired high resolution IR spectra of CI Tau, the host star of one of the few young planet candidates amenable to direct spectroscopic detection. We confirm the planet's existe…

astro-ph.SR201925 cited

Effective Temperatures of Low-Mass Stars from High-Resolution H-band Spectroscopy

Ricardo López-Valdivia, Gregory N. Mace, Kimberly R. Sokal +9

High-resolution, near-infrared spectra will be the primary tool for finding and characterizing Earth-like planets around low-mass stars. Yet, the properties of exoplanets can not b…