activity
20202026
most citedEvolution of the Exoplanet Size Distribution: Forming Large Super-Earths Over Billions of Years

56 citations · 442 across the 52 of their papers we have counts for

collaborators
Showing 2024Show all

11 papers · 1 filter

astro-ph.SR2024★ 6 cited

ChronoFlow: A Data-Driven Model for Gyrochronology

Phil R. Van-Lane, Joshua S. Speagle, Gwendolyn M. Eadie +6

Gyrochronology is a technique for constraining stellar ages using rotation periods, which change over a star's main sequence lifetime due to magnetic braking. This technique shows…

astro-ph.GA2024

The temporal and spatial variations of lithium abundance in the Galactic disc

Tiancheng Sun, Shaolan Bi, Xunzhou Chen +7

This study investigates the temporal and spatial variations in lithium abundance within the Milky Way using a sample of 22,034 main-sequence turn-off (MSTO) stars and subgiants, ch…

astro-ph.GA2024

When LAMOST meets Gaia DR3 Exploring the metallicity of open clusters

R. Zhang, Guo-Jian Wang, Yuxi +9

Context. Open clusters (OCs) are valuable probes of stellar population characteristics. Their age and metallicity provide insights into the chemical enrichment history of the Milky…

astro-ph.SR2024

The Dog that Didn't Bark: Non-Variable Field Stars in the RR Lyrae Instability Strip

Yuxi Lu, Cecilia Mateu, K. Z. Stanek

RR Lyrae stars (RRLs) are easy to identify thanks to their large photometric variation and short periods. All stars in the RRL instability strip are pulsators is often a hidden ass…

astro-ph.SR2024

On Convective Turnover Times and Dynamos In Low-Mass Stars

Seth Gossage, Rocio Kiman, Kristina Monsch +7

The relationship between magnetic activity and Rossby number is one way through which stellar dynamos can be understood. Using measured rotation rates and X-ray to bolometric lumin…

astro-ph.GA2024★ 1 cited

The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars are Metal-Rich

James W. Johnson, David H. Weinberg, Guillermo A. Blanc +12

Metallicities of both gas and stars decline toward large radii in spiral galaxies, a trend known as the radial metallicity gradient. We quantify the evolution of the metallicity gr…

astro-ph.SR2024

Evidence of Truly Young high- Dwarf Stars

Yuxi Lu, Isabel L. Colman, Maryum Sayeed +14

The existence of high- stars with inferred ages < 6 Gyr has been confirmed recently with large spectroscopic and photometric surveys. However, stellar mergers or binary interact…

astro-ph.SR2024

The impact of stellar metallicity on rotation and activity evolution in the Kepler field using gyro-kinematic ages

Victor See, Yuxi, Lu +2

In recent years, there has been a push to understand how chemical composition affects the magnetic activity levels of main sequence low-mass stars. Results indicate that more metal…

astro-ph.SR2024★ 4 cited

zoomies: A tool to infer stellar age from vertical action in Gaia data

Sheila Sagear, Adrian M. Price-Whelan, Sarah Ballard +4

Stellar age measurements are fundamental to understanding a wide range of astronomical processes, including Galactic dynamics, stellar evolution, and planetary system formation. Ho…

astro-ph.GA2024★ 1 cited

Stellar Mergers or Truly Young? Intermediate-Age Stars on Highly-Radial Orbits in the Milky Way's Stellar Halo

Danny Horta, Yuxi, Lu +3

Reconstructing the mass assembly history of the Milky Way relies on obtaining detailed measurements of the properties of many stars in the Galaxy, especially in the stellar halo. O…

astro-ph.SR2024★ 1 cited

Methods for the detection of stellar rotation periods in individual TESS sectors and results from the Prime mission

Isabel L. Colman, Ruth Angus, Trevor David +3

For ongoing studies of the role of rotation in stellar evolution, we require large catalogs of rotation periods for testing and refining gyrochronology. While there is a wealth of…