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Ray Weymann is a retired astronomer and as … Ray Weymann is a retired astronomer and astrophysicist, associated with the Carnegie Institution of Washington. His PhD is from Princeton University. He is a founder of the Climate Science Rapid Response Team, a member National Academy of Sciences (1984), and past president of the Astronomical Society of the Pacific 1973-1975. He has made notable contributions to astronomy in the areas of the evolution of high redshift galaxies, and mass ejection from active galaxies.s, and mass ejection from active galaxies.
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http://www.worldcat.org/title/heating-of-stellar-chromospheres-by-shock-waves-and-coronal-evaporation-as-a-possible-mechanism-for-mass-loss-in-red-giants/oclc/79363754&referer=brief_results +
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Heating of stellar chromospheres by shock waves and coronal evaporation as a possible mechanism for mass loss in red giants.
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http://www.worldcat.org/title/heating-of-stellar-chromospheres-by-shock-waves-and-coronal-evaporation-as-a-possible-mechanism-for-mass-loss-in-red-giants/oclc/79363754&referer=brief_results +
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Ray Weymann is a retired astronomer and as … Ray Weymann is a retired astronomer and astrophysicist, associated with the Carnegie Institution of Washington. His PhD is from Princeton University. He is a founder of the Climate Science Rapid Response Team, a member National Academy of Sciences (1984), and past president of the Astronomical Society of the Pacific 1973-1975. He has made notable contributions to astronomy in the areas of the evolution of high redshift galaxies, and mass ejection from active galaxies.s, and mass ejection from active galaxies.
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Ray Weymann
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