Pulsar timing irregularities and the imprint of magnetic field evolution

Astronomy and Astrophysics

Volumn 547, Issue , 2012, Pages

  Pons, J A ^a   Vigano D ^a   Geppert, U ^b,c  

^a UNIVERSITY OF ALICANTE   (Spain)

^b GERMAN AEROSPACE CENTER DLR   (Germany)

^c UNIVERSITY OF ZIELONA GÓRA   (Poland)

Author keywords

Pulsars: general; Stars: evolution; Stars: magnetic field; Stars: neutron

Indexed keywords

ABSOLUTE VALUES; AXISYMMETRIC; CRUSTAL FIELDS; DIPOLAR FIELDS; EVOLUTION MODELS; FIELD DECAYS; FIELD EVOLUTION; FIELD STRUCTURES; INDEX N; INTERIOR TEMPERATURE; INTERNAL TEMPERATURE; ISOLATED NEUTRON STARS; LONG TERM SIMULATION; LOW FIELD; MAGNETIC FIELD MODIFICATION; NEUTRON STARS; OHMIC DISSIPATION; OSCILLATORY MODE; PULSARS: GENERAL; SMALL VARIATIONS; STARS: EVOLUTION; STARS: MAGNETIC FIELD; STARS: NEUTRONS; SUPERNOVA EXPLOSION; TEMPORAL VARIATION; TIME-SCALES; TIMING NOISE; TIMING PROPERTIES; TOROIDAL COMPONENTS;

MAGNETIC FIELDS; MAGNETOS; NEUTRONS;

STARS;

EID: 84867640730     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220091     Document Type: Article

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