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nstitute a very revealing source of information. A spectrometry of its light can disclose, to be sure, the temperature (colour, or ionization) of the star‘s semi-transparent outer layers, their chemical composition, and prevalent pressure (through Stark effect) or magnetic field (Zeeman effect), it

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Bruce Waxman BMedSc., MBBS, FRACS, FRCS(eng), FACS,Brendon J. Coventry BMBS, PhD, FRACS, FACS, FRSMcaused by eclipses in the time-domain. Unfortunately, a transcendental character of its dependence on . and . has made it impossible to construct a mathematical solution of the underlying problem otherwise than by successive approximations; and no one succeeded so far to express this function analyt

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Bruce Waxman MBBS, FRACS, FRCS(eng), FACS,Brendon J. Coventry BMBS, PhD, FRACS, FACS, FRSM of language. Offering an antidote to the current thinking embracing ‘biologism’ in linguistic sciences, it will be of interest to readers in linguistics, the cognitive and brain sciences, and the points at whi978-3-030-23717-2978-3-030-23715-8

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Bruce Waxman MBBS, FRACS, FRCS(eng), FACS,Brendon J. Coventry BMBS, PhD, FRACS, FACS, FRSM,David Wathe inter­ pretation of the observed light changes of eclipsing binary stars and their analysis for the elements of the respective systems. Whenever we study the properties of any celestial body - be it a planet or a star - all information we wish to gain can reach us through two different channels: