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

Bellinger, E. P.; Hekker, Saskia; Angelou, George C.; Stokholm, A.; Basu, S.

doi:10.1051/0004-6361/201834461e

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

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

MPS-Authors

/persons/resource/persons123110

Hekker, Saskia
Max Planck Research Group in Stellar Ages and Galactic Evolution (SAGE), Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons140524

Angelou, George C.
Max Planck Research Group in Stellar Ages and Galactic Evolution (SAGE), Max Planck Institute for Solar System Research, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

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.

Cite as: https://hdl.handle.net/21.11116/0000-0006-F53F-0

Abstract

There is no abstract available