On the distribution of intensity in stellar absorption lines

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About this book

"On the Distribution of Intensity in Stellar Absorption Lines" by Payne-Gaposchkin et al. is a scientific publication written in the early 20th century. This work focuses on the quantitative analysis of the intensity and contours of absorption lines observed in the spectra of various stars, utilizing observational data and new measurement techniques. The document is technical in nature and is intended for readers with a background in astrophysics or astronomy, particularly those interested in stellar atmospheres and spectral analysis. The opening of this publication introduces the significance of studying stellar absorption lines for understanding atomic structure and star atmospheres, while noting a gap between theory and quantitative observation. The authors then outline their methodology: employing the Harvard Observatory's 16-inch refractor with objective prisms and specialized apertures to record spectra of eleven stars across different spectral types.