Eddington's theory appeared in mature form in 1926 as The Internal Constitution of the Stars, which became an important text for training an entire generation of astrophysicists.
Eddington julkaisi teoriansa kehitetyssä muodossa vuonna 1926 teoksessaan The Internal Constitution of the Stars, josta tuli tärkeä tietolähde kokonaiselle astrofyysikkojen sukupolvelle.