Titlebook: Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems; Thomas B. Ake,Elizabeth Griffin Book 2015 Springer International Publishi

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Tanja Klenk,Frank Nullmeier,Göttrik Wewerthe system and components, a high-mass versus low-mass model dilemma persists. This chapter examines some of the recent developments and attempts to place the system among the pantheon of binary types. It also offers suggestions for observational tests prior to the next eclipse in 2037.

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, Aurigae: A Two Century Long Dilemma Persists,the system and components, a high-mass versus low-mass model dilemma persists. This chapter examines some of the recent developments and attempts to place the system among the pantheon of binary types. It also offers suggestions for observational tests prior to the next eclipse in 2037.

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Achim Kießig,Katja Lohmann,Cornelia Zanger data that have been used in those analyses, and examines each of the 10 known eclipsing systems in turn, except for VV Cep which is treated separately in Chap. . It describes what has been achieved by modelling, and assesses what has been learned so far about the mass loss and winds from the cool g

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Handbuch Digitaler Schnittstellension to what can be learned by eclipse mapping, but are fraught with many challenges. The space-UV absorption spectrum is extremely rich, and line blending is severe. Wind interaction and accretion effects are prominent, and the spectrum of the B star companion is heavily veiled by overlying Balmer

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Living reference work 20200th edition, show extended and highly turbulent chromospheres, which develop into slow massive winds. The associated continuous mass loss has a significant impact on stellar evolution, and thence on the chemical evolution of galaxies. Yet despite the fundamental importance of those winds in astrophysics, the q

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