File:Hubble’s Views of M13 (2010) and M3 (2019).jpg
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Summary
DescriptionHubble’s Views of M13 (2010) and M3 (2019).jpg |
English: To investigate the physics underpinning white dwarf evolution, astronomers compared cooling white dwarfs in two massive collections of stars: the globular clusters M3 and M13. These two clusters share many physical properties such as age and metallicity but the populations of stars which will eventually give rise to white dwarfs are different. This makes M3 and M13 together a perfect natural laboratory in which to test how different populations of white dwarfs cool. |
Date | |
Source | https://esahubble.org/images/heic2108a/ |
Author | ESA/Hubble & NASA, G. Piotto et al. |
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This file is licensed under the Creative Commons Attribution 4.0 International license.
Attribution: ESA/Hubble
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 20:49, 28 September 2021 | 6,182 × 3,116 (10.09 MB) | Pandreve | Uploaded a work by ESA/Hubble & NASA, G. Piotto et al. from https://esahubble.org/images/heic2108a/ with UploadWizard |
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Image title |
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Source | ESA/Hubble |
Credit/Provider | ESA/Hubble & NASA, G. Piotto et al. |
Short title |
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Usage terms |
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Date and time of data generation | 17:00, 6 September 2021 |
JPEG file comment | To investigate the physics underpinning white dwarf evolution, astronomers compared cooling white dwarfs in two massive collections of stars: the globular clusters M3 and M13. These two clusters share many physical properties such as age and metallicity but the populations of stars which will eventually give rise to white dwarfs are different. This makes M3 and M13 together a perfect natural laboratory in which to test how different populations of white dwarfs cool. |
Software used | Adobe Photoshop 22.4 (Windows) |
File change date and time | 19:07, 21 August 2021 |
Date and time of digitizing | 21:04, 21 August 2021 |
Date metadata was last modified | 21:07, 21 August 2021 |
Unique ID of original document | xmp.did:be09bcff-d104-2b42-ab66-ba7135cbb411 |
Keywords |
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Contact information |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
IIM version | 4 |