Stellar ages, masses, and radii from asteroseismic modeling are robust to systematic errors in spectroscopy (Corrigendum)

This item is discarded!DetailsSummary

Stellar ages, masses, and radii from asteroseismic modeling are robust to systematic errors in spectroscopy (Corrigendum)

Bellinger, E. P., Hekker, S., Angelou, G. C., Stokholm, A., & Basu, S. (2020). Stellar ages, masses, and radii from asteroseismic modeling are robust to systematic errors in spectroscopy (Corrigendum). Astronomy and Astrophysics, 635: C2. doi:10.1051/0004-6361/201834461e.

Item is Discarded

Basic (Discarded)

Date of Discard: 2020-11-04

Comment: Dublette

Creators:
Bellinger, E. P.
Hekker, Saskia¹
Angelou, G. C.¹
Stokholm, A.
Basu, S.

Affiliations:
1Max Planck Research Group in Stellar Ages and Galactic Evolution (SAGE), Max Planck Institute for Solar System Research, Max Planck Society, ou_2265636

Dates: Published Online: 2020

Files: 0 Files

Locators: 0 Locators

version ID: item_3253530_1

Item State: Discarded

Name of Context: Publications of the MPI for Solar System Research, Affiliated to: Max Planck Institute for Solar System Research