Correction: Cuello, N.; Sucerquia, M. Alpha Centauri: Disc Dynamics, Planet Stability, Detectability. Universe 2024, 10, 64
1
Univ. Grenoble Alpes, CNRS, IPAG, 38000 Grenoble, France
2
UFR PHysique, Ingénierie, Terre, Environnement, Mécanique de l’Université de Grenoble Alpes, France
3
Departamento de Ciencias, Facultad de Artes Liberales, Universidad Adolfo Ibáñez, Av. Padre Hurtado 750, Viña del Mar 2520000, Chile
4
Núcleo Milenio Formación Planetaria—NPF, Universidad Adolfo Ibáñez, Av. Padre Hurtado 750, Viña del Mar 2520000, Chile
*
Authors to whom correspondence should be addressed.
†
These authors contributed equally to this work.
Universe 2024, 10(3), 120; https://doi.org/10.3390/universe10030120
Submission received: 21 February 2024
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Accepted: 22 February 2024
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Published: 4 March 2024
(This article belongs to the Special Issue The Royal Road: Eclipsing Binaries and Transiting Exoplanets)
In the original publication [1], there was a mistake in Figure A2 as published. The sub-figures were the same, but the sub figure Alpha Cen B should be different from Alpha Cen A. The corrected Figure A2 appears below. The authors state that the scientific conclusions are unaffected. This correction was approved by the Academic Editor. The original publication has also been updated.
Reference
- Cuello, N.; Sucerquia, M. Alpha Centauri: Disc Dynamics, Planet Stability, Detectability. Universe 2024, 10, 64. [Google Scholar] [CrossRef]
Figure A2.
Stability maps based on MEGNO values for test particles around Alpha Cen A (left panel) and Alpha Cen B (right panel) over a 100,000-year period for a 20 × 20 grid in the a–e parameter space. Dynamically stable regions are coloured in blue.
Figure A2.
Stability maps based on MEGNO values for test particles around Alpha Cen A (left panel) and Alpha Cen B (right panel) over a 100,000-year period for a 20 × 20 grid in the a–e parameter space. Dynamically stable regions are coloured in blue.
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MDPI and ACS Style
Cuello, N.; Sucerquia, M. Correction: Cuello, N.; Sucerquia, M. Alpha Centauri: Disc Dynamics, Planet Stability, Detectability. Universe 2024, 10, 64. Universe 2024, 10, 120. https://doi.org/10.3390/universe10030120
AMA Style
Cuello N, Sucerquia M. Correction: Cuello, N.; Sucerquia, M. Alpha Centauri: Disc Dynamics, Planet Stability, Detectability. Universe 2024, 10, 64. Universe. 2024; 10(3):120. https://doi.org/10.3390/universe10030120
Chicago/Turabian StyleCuello, Nicolás, and Mario Sucerquia. 2024. "Correction: Cuello, N.; Sucerquia, M. Alpha Centauri: Disc Dynamics, Planet Stability, Detectability. Universe 2024, 10, 64" Universe 10, no. 3: 120. https://doi.org/10.3390/universe10030120
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