A highly resistive layer within the crust of X-ray pulsars limits their spin periods
Jose A. Pons · Daniele Viganò · Nanda Rea
Apr 25, 2013#9*↳ astro-ph.SRNat.Phys.149 citations
Author
Viganò, Daniele Maria
INSPIRE profile1241906ORCID0000-0001-7795-6850
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