activity
20172020
most citedHigh-precision abundances of elements in solar-type stars. Evidence of two distinct sequences in abundance-age relations

124 citations · 381 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2020124 cited

High-precision abundances of elements in solar-type stars. Evidence of two distinct sequences in abundance-age relations

P. E. Nissen, J. Christensen-Dalsgaard, J. R. Mosumgaard +3

HARPS spectra with signal-to-noise ratios S/N > 600 at 6000 A were analysed with MARCS model atmospheres to obtain 1D LTE abundances of C, O, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni, Sr…

astro-ph.GA202084 cited

Age dating of an early Milky Way merger via asteroseismology of the naked-eye star Indi

William J. Chaplin, Aldo M. Serenelli, Andrea Miglio +81

Over the course of its history, the Milky Way has ingested multiple smaller satellite galaxies. While these accreted stellar populations can be forensically identified as kinematic…

astro-ph.SR201954 cited

Detection and characterisation of oscillating red giants: first results from the TESS satellite

Víctor Silva Aguirre, Dennis Stello, Amalie Stokholm +78

Since the onset of the `space revolution' of high-precision high-cadence photometry, asteroseismology has been demonstrated as a powerful tool for informing Galactic archaeology in…

astro-ph.SR2019

The subgiant HR 7322 as an asteroseismic benchmark star

Amalie Stokholm, Poul Erik Nissen, Victor Silva Aguirre +5

We present an in-depth analysis of the bright subgiant HR 7322 (KIC 10005473) using Kepler short-cadence photometry, optical interferometry from CHARA, high-resolution spectra from…

astro-ph.EP201995 cited

A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS

Daniel Huber, William J. Chaplin, Ashley Chontos +139

We present the discovery of TOI-197.01, the first transiting planet identified by the Transiting Exoplanet Survey Satellite (TESS) for which asteroseismology of the host star is po…

astro-ph.SR2018

Helium abundance in a sample of cool stars: measurements from asteroseismology

Kuldeep Verma, Keyuri Raodeo, Sarbani Basu +5

The structural stratification of a solar-type main sequence star primarily depends on its mass and chemical composition. The surface heavy element abundances of the solar-type star…