Abstract
We shall begin with a discussion of our nearest star, the Sun. In Sect. 6.1, we collect the data concerning the Sun, which are often used to define units for describing the properties of other stars, and introduce the energy distribution of the solar radiation from the photosphere: a continuum with numerous absorption lines.
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Unsöld, A., Baschek, B. (2002). The Distances and Fundamental Properties of the Stars. In: The New Cosmos. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-04356-1_6
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DOI: https://doi.org/10.1007/978-3-662-04356-1_6
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