File:HR 6819 illustration.jpg
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editDescriptionHR 6819 illustration.jpg |
English: Schematic illustration of the observations and competing scenarios for HR 6819. Sizes and distances are not to scale. Top: spectroscopic observations. Middle: original scenario, with a giant B star orbiting a black hole, and a rapidly-spinning Be star further away. Bottom: alternative scenario without a black hole,with a stripped B star that is less massive than the Be one. Note that the spectral lines of the Be star do wobble very slightly (not shown here). |
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Date | 28 February 2022, 17:26 | ||||
Source | https://www.eso.org/public/images/black-hole-rebuttal/ | ||||
Author | ESO/J. C. Munoz-Mateos, D. Catricheo | ||||
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current | 18:29, 2 December 2023 | 16,667 × 16,667 (6.26 MB) | Юрий Д.К. (talk | contribs) | {{Information |description={{en|1=Schematic illustration of the observations and competing scenarios for HR 6819. Sizes and distances are not to scale. Top: spectroscopic observations. Middle: original scenario, with a giant B star orbiting a black hole, and a rapidly-spinning Be star further away. Bottom: alternative scenario without a black hole,with a stripped B star that is less massive than the Be one. Note that the spectral lines of the Be star do wobble very slightly (not shown here).}... |
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Image title |
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Credit/Provider | ESO/J. C. Munoz-Mateos, D. Catricheo |
Source | European Southern Observatory |
Short title |
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Usage terms |
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Date and time of data generation | 17:26, 28 February 2022 |
Software used | Adobe InDesign 16.4 (Macintosh) |
File change date and time | 12:12, 28 February 2022 |
Date and time of digitizing | 13:09, 28 February 2022 |
Date metadata was last modified | 13:12, 28 February 2022 |
Unique ID of original document | xmp.did:56749111-5132-4425-b865-67d42848c259 |
Contact information |
Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |
IIM version | 4 |