File:Distributions of metallicity and abundance ratios (geminiann13002b).jpg
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Distributions_of_metallicity_and_abundance_ratios_(geminiann13002b).jpg (500 × 319 pixels, file size: 63 KB, MIME type: image/jpeg)
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Distributions of metallicity [M/H] and abundance ratios [α/Fe] for each of the clusters derived from the line indices. Under the assumption of passive evolution there should not be any significant differences from cluster to cluster.
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[edit]DescriptionDistributions of metallicity and abundance ratios (geminiann13002b).jpg |
English: Distributions of metallicity [M/H] and abundance ratios [α/Fe] for each of the clusters derived from the line indices. Under the assumption of passive evolution there should not be any significant differences from cluster to cluster. Instead we find that MS0451.6-0305 has [M/H] about 0.2 dex below that of the other clusters, while RXJ0152.7-1237 has [α/Fe] about 0.3 dex above that of the other clusters. |
Date | 1 February 2013, 15:28:00 (upload date) |
Source | Distributions of metallicity and abundance ratios |
Author | NOIRLab/Gemini Observatory/AURA |
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current | 18:24, 23 October 2023 | ![]() | 500 × 319 (63 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/geminiann13002b.jpg via Commons:Spacemedia |
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Credit/Provider | NOIRLab/Gemini Observatory/AURA |
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Source | NSF's NOIRLab |
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Date and time of data generation | 15:28, 1 February 2013 |
Software used | Adobe Photoshop 21.2 (Windows) |
File change date and time | 15:29, 27 July 2020 |
Date and time of digitizing | 01:32, 30 January 2013 |
Date metadata was last modified | 10:29, 27 July 2020 |
Unique ID of original document | uuid:6EF346DE626CE211868FA24538C7EB9A |
Copyright status | Copyright status not set |
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IIM version | 4 |