Research ArticleASTRONOMY

Magnetar formation through a convective dynamo in protoneutron stars

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Science Advances  13 Mar 2020:
Vol. 6, no. 11, eaay2732
DOI: 10.1126/sciadv.aay2732

Article Information

vol. 6 no. 11

Online ISSN: 
History: 
  • Received for publication June 4, 2019
  • Accepted for publication December 17, 2019
  • .

Author Information

  1. Raphaël Raynaud1,*,
  2. Jérôme Guilet1,
  3. Hans-Thomas Janka2 and
  4. Thomas Gastine3
  1. 1AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France.
  2. 2Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85748 Garching, Germany.
  3. 3Institut de Physique du Globe de Paris, Sorbonne Paris Cité, Université Paris-Diderot, UMR7154 CNRS, 1 rue Jussieu, 75005 Paris, France.
  1. *Corresponding author. Email: raphael.raynaud{at}cea.fr

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