In this paper I discuss how awareness of the existence of white dwarfs developed in conjunction with an improved understanding of the nature of the Sun and the stars, as well as how it involved the efforts of a number of astronomers, both observers and theoreticians. I review some of the key discoveries and insights that led to a final acceptance of the reality of `white dwarfs', including the actual origin of the term itself. The observations that I primarily draw upon involve the faint blue companions of the nearby stars ?2 Eridani (40 Eri) and Sirius. As will be seen, the subluminous character of both companions was evident long before it was widely appreciated how truly unusual these stars actually are. Although there are several prior reviews of the early history of white dwarfs, including a brief but comprehensive one by Hearnshaw,1 the present paper provides a thorough overview of this subject.
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