About: Ray Weymann

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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.

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  • 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. (en)
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  • Heating of stellar chromospheres by shock waves and coronal evaporation as a possible mechanism for mass loss in red giants. (en)
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  • 1960 (xsd:integer)
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  • 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. (en)
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  • Ray Weymann (en)
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