File:Second parameter problem.png
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![File:Second parameter problem.png](https://upload.wikimedia.org/wikipedia/commons/thumb/3/36/Second_parameter_problem.png/600px-Second_parameter_problem.png?20210312181429)
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Metallicity — blueness diagram for some globular clusters, illustrating the second parameter problem
Диграмма металличность — голубизна для шаровых скоплений, иллюстрирующая проблему второго параметра
Summary
[edit]DescriptionSecond parameter problem.png |
English: Metallicity — blueness diagram for some globular clusters, illustrating the second parameter problem. Blueness depends of horizontal branch morphology and equals number of stars bluer than RR Lyrae stars minus number of stars redder than RR Lyrae, divided on number of stars on horizontal branch.
This diagram is a reproduction of the similar one from this website: http://heritage.sai.msu.ru/ucheb/Samus/2_5.html
Русский: Диграмма металличность — голубизна для шаровых скоплений, иллюстрирующая проблему второго параметра. Голубизна — параметр, зависящий от морфологии горизонтальной ветви и равный разности звёзд на голубом и красном конце горизонтальной ветви, делённой на общее количество звёзд на горизонтальной ветви.
Эта диаграмма является репродукцией аналогичной с этого сайта: http://heritage.sai.msu.ru/ucheb/Samus/2_5.html |
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Author | Vallastro |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 18:14, 12 March 2021 | ![]() | 1,152 × 1,152 (54 KB) | Vallastro (talk | contribs) | Font size increased (again) |
15:40, 12 March 2021 | ![]() | 1,152 × 1,152 (41 KB) | Vallastro (talk | contribs) | Font size increased | |
12:06, 23 February 2021 | ![]() | 1,025 × 969 (23 KB) | Vallastro (talk | contribs) | Uploaded own work with UploadWizard |
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