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Titlebook: Hydrodynamics and Stellar Winds; An Introduction Walter J. Maciel Textbook 2014 Springer Nature Switzerland AG 2014 Astrophysical fluid equ

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Hydrodynamics and Stellar Winds978-3-319-04328-9Series ISSN 2192-4791 Series E-ISSN 2192-4805
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Sound Waves,peed of sound. A discussion is given on the existence of a critical point in the solution of the hydrodynamic equations in stellar winds in the isothermal case. The general topology of the possible solutions is presented and some consequences on the stellar mass loss rate are discussed.
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David A. Kopriva,Edwin Jimenez noted that there are many topics which I have not covered but which should form part of a more complete survey. Among topics which merit proper discussion I would include the re-ionisation of the intergalactic gas, the nature of the absorption line systems observed in distant quasars and their role
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Systems over a Semiring: Realization and Decouplingn networks, and manufacturing systems. This paper generalizes the original system theory invented by R. E. Kalman for traditional linear systems. Kalman constructed the “state” module, the input/output map, and a canonical realization in terms of reachability and observability. The advantage of this
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