Differences between the two anomalous X-ray pulsars: Variations in the spin-down rate of IE 1048.1-5937 and an extended interval of quiet spin-down in IE 2259+586

Monthly Notices of the Royal Astronomical Society

Volumn 319, Issue 1, 2000, Pages 205-208

  Baykal, Altan ^a   Strohmayer, Tod ^d   Swank, Jean ^d   Alpar, M Ali ^b   Stark, Michael J ^c  

^a MIDDLE EAST TECHNICAL UNIVERSITY   (Turkey)

^b SABANCI UNIVERSITY   (Turkey)

^c DENISON UNIVERSITY   (United States)

^d NONE

Author keywords

Accretion, accretion discs; Binaries: general; Stars: individual: 1E 1048.1 5937; Stars: individual: 1E 2259+586; Stars: low mass, brown dwarfs

Indexed keywords

LUMINANCE;

ACCRETION: ACCRETION DISKS; BINARIES:GENERAL; SPIN-DOWN; STAR: INDIVIDUAL: 1E 1048.1-5937; STAR: INDIVIDUAL: 1E 2259+586; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: LOW-MASS BROWN DWARFS; X-RAY LUMINOSITY; X-RAY TIMING EXPLORERS;

PULSARS;

EID: 0008610318     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03845.x     Document Type: Article

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