Die Rotverschiebung von extragalaktischen Nebeln (Scholarly article) (Q1556): Difference between revisions
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Adding Zwicky 1933 scholarly article. |
Linked Die Rotverschiebung von extragalaktischen Nebeln (Scholarly article) to its wiki page |
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| Property / page(s): 110–127 / rank | |||||||||||||||
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| Property / journal (entity): Helvetica Physica Acta / rank | |||||||||||||||
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| Property / date: 1933 / rank | |||||||||||||||
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| Property / access URL: https://ui.adsabs.harvard.edu/abs/1933AcHPh...6..110Z/abstract / rank | |||||||||||||||
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| Property / attributed to: Fritz Zwicky / rank | |||||||||||||||
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1933
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Latest revision as of 08:07, 3 September 2026
1933 paper by Fritz Zwicky on the redshifts of extragalactic nebulae: applying the virial theorem to the Coma cluster he found its galaxies move too fast for the visible mass, inferring the presence of large amounts of non-luminous ("dark") matter, usually cited as the first evidence for dark matter
| Language | Label | Description | Also known as |
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| English | Die Rotverschiebung von extragalaktischen Nebeln (Scholarly article) |
1933 paper by Fritz Zwicky on the redshifts of extragalactic nebulae: applying the virial theorem to the Coma cluster he found its galaxies move too fast for the visible mass, inferring the presence of large amounts of non-luminous ("dark") matter, usually cited as the first evidence for dark matter |
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110–127
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6
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1933
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