Observational Constraints to the Evolution of Massive Stars
classification
🌌 astro-ph
keywords
massivestarsevolutionregionsaspectsconsiderconstraintsdetail
read the original abstract
We consider some aspects of the evolution of massive stars which can only be elucidated by means of "indirect" observations, i.e. measurements of the effects of massive stars on their environments. We discuss in detail the early evolution of massive stars formed in high metallicity regions as inferred from studies of HII regions in external galaxies.
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.