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Magnetar formation through a convective dynamo in protoneutron stars

The release of spin-down energy by a magnetar is a promising scenario to power several classes of extreme explosive transients. However, it lacks a firm basis because magnetar formation still represents a theoretical challenge. Using the first three-dimensional simulations of a convective dynamo bas...

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Detalles Bibliográficos
Autores principales: Raynaud, Raphaël, Guilet, Jérôme, Janka, Hans-Thomas, Gastine, Thomas
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2020
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7069699/
https://www.ncbi.nlm.nih.gov/pubmed/32201719
http://dx.doi.org/10.1126/sciadv.aay2732