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In this interview, Geoffrey Burbidge discusses his life and career. Topics discussed include: his family and childhood; Bristol University; Nevill Mott; University College, London; Harrie Massey; David Robert Bates; theoretical physics seminars at Cambridge University; Richard Feymnan; Freeman Dyson; Dick Dalitz; Abdus Salam; Nicholas Kemmer; becoming interested in astronomy and astrophysics via Margaret Burbidge; Royal Astronomical Society; Clive Gregory; research into stellar parallax, stellar atmospheres; Herbert Dingle; Auger effect; Otto Struve; Harvard University; Bart Bok; Donald Menzel; Harlow Shapley; Yerkes Observatory; development of radio astronomy; I. I. Rabi and big bang skepticism; Chandrasekhar; Gerard Kuiper; Enrico Fermi; Cavendish Laboratory, Martin Ryle; nucleosynthesis; Kapitza Club; Willie Fowler; Fred Hoyle; stellar evolution; steady state cosmology; red shift; Erwin Finlay-Freundlich; Max Born; Mount Wilson Observatory; Allan Sandage; Milt Humason; Ira Bowen; status at women at Hale observatories and at the California Institute of Technology (CalTech); Edwin Hubble; Walter Baade; synchrotron radiation; Rudolph Minkowski; Californium and supernovae; Halton Arp; Hans Suess; Vera Rubin's work on anisotropy; quasars; galaxy formation.
Discusses her childhood and education; her developing interest in astronomy; studying with C. C. L. Gregory at the University of London Observatory and University College; her thesis work on the variations in Gamma Cassiopeia; meeting and marrying Geoffrey Burbidge; discrimination against women in the Carnegie Followships; the conflict between her work and having a family; the decision to go to the U.S. and Yerkes; use of the 82-inch telescope at McDonald; recollections of Shapley; disagreements between Kuiper and Urey; development of interest in abundance of elements; Baade's inspiration; offers for Geoffrey Burbidge from Manchester and Cambridge and move to Cambridge University; Geoffrey's differences with M. Ryle involving source of radio emission; meeting Willie Fowler; decision to return to the U. S. and Caltech; observing time at Mt Wilson; reactions of the old guard to women observers; collaborations with Baade on supernovae synthesis (1956); work on barium II stars; the search for permanent positions; advantage of position at Chicago/Yerkes/McDonald; move to Chicago and work on galaxies (1957-1962); observations of Centaurus A at 82-inch McDonald telescope; leaving Yerkes to go to La Jolla with Revelle; continued research on quasars and general research; cosmological implications of quasars; summer in Pasadena with Hoyle; development of Hoyle's Institute; challenges of Burbidge, Fowler, Hoyle concept of nucleosynthesis; Unsold's arguments; Arp's work; lack of satisfactory gravitational red shift models; university's relationship with Lick; infra-red work future of Greenwich and changes in the power structure in the British Astronomical establishment; offer of position as head of the Science Research Council; decision to take a leave of absence from La Jolla and accept; difficulties of the position and the decision as to where to locate the Northern Hemisphere Observatory; decision to return to the U. S.; American Astronomical Society presidency (1976-1978); AAS and the Equal Rights Amendment; her most satisfying work in nucleosynthesis, B2FH. Among those prominently mentioned: Arp, Baade, Bowen, Chandrasekhar, Greenstein, Hoyle, Kuiper, P. Merrill, H. Minkowski, R. Revelle, M. Ryle, Sandage, Shapley, Stromgren, Unsold, Urey.