activity
19982026
most citedHelioseismology and Solar Abundances

422 citations · 3.3k across the 76 of their papers we have counts for

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Showing 2020Show all

17 papers · 1 filter

astro-ph.SR20204 cited

Inverse analysis of asteroseismic data: a review

Earl P. Bellinger, Sarbani Basu, Saskia Hekker

Asteroseismology has emerged as the best way to characterize the global and internal properties of nearby stars. Often, this characterization is achieved by fitting stellar evoluti…

astro-ph.GA202050 cited

Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the Continuous Viewing Zones and beyond

J. Ted Mackereth, Andrea Miglio, Yvonne Elsworth +30

The NASA- mission presents a treasure trove for understanding the stars it observes and the Milky Way, in which they reside. We present a first look at the prospects for…

astro-ph.SR202019 cited

Differential Modelling Systematics across the HR Diagram from Asteroseismic Surface Corrections

J. M. Joel Ong, Sarbani Basu, Jean M. McKeever

Localised modelling error in the near-surface layers of evolutionary stellar models causes the frequencies of their normal modes of oscillation to differ from those of actual stars…

astro-ph.SR2020

Solar Cycle Related Changes in the Helium Ionization Zones of the Sun

Courtney B. Watson, Sarbani Basu

Helioseismic data for solar cycles 23 and 24 have shown unequivocally that solar dynamics changes with solar activity. Changes in solar structure have been more difficult to detect…

astro-ph.SR2020

Robust asteroseismic properties of the bright planet host HD 38529

Warrick H. Ball, William J. Chaplin, Martin B. Nielsen +21

The Transiting Exoplanet Survey Satellite (TESS) is recording short-cadence, high duty-cycle timeseries across most of the sky, which presents the opportunity to detect and study o…

astro-ph.SR2020

Examining the Relationship Between Convective Core Overshoot and Stellar Properties Using Asteroseismology

Lucas S. Viani, Sarbani Basu

Core overshoot is a large source of uncertainty in constructing stellar models. Whether the amount of overshoot is constant or mass dependent is not completely known, even though m…