
Sign up to save your podcasts
Or
In this episode Dr Ezzeddine told me about how the chemical and physical compositions of stars can be inferred by the use of spectroscopy. Additionally, she explained what the r-process is, and how by building radiative transfer models we can calculate the abundances of elements in the atmospheres of stars.
5
55 ratings
In this episode Dr Ezzeddine told me about how the chemical and physical compositions of stars can be inferred by the use of spectroscopy. Additionally, she explained what the r-process is, and how by building radiative transfer models we can calculate the abundances of elements in the atmospheres of stars.