Neutron star glitches have a substantial minimum size

Monthly Notices of the Royal Astronomical Society

Volumn 440, Issue 3, 2014, Pages 2755-2762

  Espinoza, C M ^a,b   Antonopoulou, D ^c   Stappers, B W ^a   Watts, A ^c   Lyne, A G ^a  

^a UNIVERSITY OF MANCHESTER   (United Kingdom)

^b PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^c UNIVERSITY OF AMSTERDAM   (Netherlands)

Author keywords

Pulsars: general; Stars: neutron

Indexed keywords

NEUTRONS;

AUTOMATED METHODS; CRAB PULSAR; DETECTABILITY; NEUTRON STARS; PULSARS: GENERAL; SPIN-DOWN; SPIN-UP; STARS: NEUTRONS; SUPERFLUID COMPONENT; THEORETICAL MODELING;

PULSARS;

EID: 84898784451     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stu395     Document Type: Article

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