activity
20172022
most citedVery regular high-frequency pulsation modes in young intermediate-mass stars

114 citations · 427 across the 10 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2022

Ages of Main-Sequence Turn-Off Stars from the GALAH Survey

Xunzhou Chen, Zhishuai Ge, Yuqin Chen +6

Main sequence turn-off (MSTO) stars are good tracers of Galactic populations since their ages can be reliably estimated from atmospheric parameters. Based on the GALAH survey, we u…

astro-ph.SR20222 cited

Modeling Stellar Oscillations and Granulation in Radial Velocity Time Series: A Fourier-based Method

Zhao Guo, Eric B. Ford, Dennis Stello +4

Tens of thousands of solar-like oscillating stars have been observed by space missions. Their photometric variability in the Fourier domain can be parameterized by a sum of two sup…

astro-ph.SR202110 cited

A binary with a ~Scuti star and an oscillating red giant: orbit and asteroseismology of KIC9773821

Simon J Murphy, Tanda Li, Sanjay Sekaran +8

We study the Scuti -- red giant binary KIC9773821, the first double-pulsator binary of its kind. It was observed by \textit{Kepler} during its four-year mission. Our aims are t…

astro-ph.SR202022 cited

Asteroseismology of luminous red giants with Kepler. II. Dependence of mass loss on pulsations and radiation

Jie Yu, Saskia Hekker, Timothy R. Bedding +5

Mass loss by red giants is an important process to understand the final stages of stellar evolution and the chemical enrichment of the interstellar medium. Mass-loss rates are thou…

astro-ph.SR2020114 cited

Very regular high-frequency pulsation modes in young intermediate-mass stars

Timothy R. Bedding, Simon J. Murphy, Daniel R. Hey +33

Asteroseismology is a powerful tool for probing the internal structures of stars by using their natural pulsation frequencies. It relies on identifying sequences of pulsation modes…

astro-ph.SR202020 cited

Solar-type Stars Observed by LAMOST and Kepler

Jinghua Zhang, Alexander I. Shapiro, Shaolan Bi +8

Obtaining measurements of chromospheric and photometric activity of stars with near-solar fundamental parameters and rotation periods is important for a better understanding of sol…