Asteroseismology of stars on the upper main sequence
classification
🌌 astro-ph.SR
keywords
mainsequencestarsupperasteroseismicasteroseismologyattentiondiagram
read the original abstract
I review the properties of pulsators located on the upper main sequence in the HR diagram and discuss asteroseismic inferences on the internal structure of stars of spectral type A and B. Special attention is given to the problem of uncertainties in stellar opacities in modelling.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.