Abstract
The systems that we shall consider primarily in this paper consist of a late-type cool supergiant or bright giant and a hot main sequence companion which periodically passes behind the larger star and shines through its extended atmosphere. This gives us the opportunity of observing absorption lines along various sightlines through the cool star’s atmosphere and hence permits us to study stratification effects and physical properties in these tenuous outer layers of the star.
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Hack, M., Stickland, D. (1987). Atmospheric Eclipses by Supergiants in Binary Systems. In: Kondo, Y., et al. Exploring the Universe with the IUE Satellite. Astrophysics and Space Science Library, vol 129. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3753-6_19
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DOI: https://doi.org/10.1007/978-94-009-3753-6_19
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