Stellar structure and compact objects before 1940: Towards relativistic astrophysics

Since the mid-1920s, different strands of research used stars as "physics laboratories" for investigating the nature of matter under extreme densities and pressures, impossible to realize on Earth. To trace this process this paper is following the evolution of the concept of a dense core in stars, which was important both for an understanding of stellar evolution and as a testing ground for the fast-evolving field of nuclear physics. In spite of the divide between physicists and astrophysicists, some key actors working in the cross-fertilized soil of overlapping but different scientific cultures formulated models and tentative theories that gradually evolved into more realistic and structured astrophysical objects. These investigations culminated in the first contact with general relativity in 1939, when J. Robert Oppenheimer and his students George Volkoff and Hartland Snyder systematically applied the theory to the dense core of a collapsing neutron star. This pioneering application of Einstein's theory to an astrophysical compact object can be regarded as a milestone in the path eventually leading to the emergence of relativistic astrophysics in the early 1960s.Comment: 83 pages, 4 figures, submitted to the European Physical Journal

The origins and abundances of the chemical elements before 1957: from Prout's hypothesis to Pasadena

The 1957 papers by Burbidge, Burbidge, Fowler, and Hoyle and by Cameron are generally regarded as the foundations upon which our modern understanding of nucleosynthesis has been erected. They were, however, also the capstones of an extended period of investigation of the composition of the cosmos (earth, sun, and beyond) and of the processes that might have given rise to that composition, dating back at least as far as 1885, that is longer before 1957 than “now” is after 1957