Evidence of a change in the long-term spin-down rate of the X-ray pulsar 4U 1907+09

Monthly Notices of the Royal Astronomical Society

Volumn 369, Issue 4, 2006, Pages 1760-1764

  Baykal, A ^a   Inam, S C ^b   Beklen, E ^a,c  

^a MIDDLE EAST TECHNICAL UNIVERSITY   (Turkey)

^b BASKENT UNIVERSITY   (Turkey)

^c SULEYMAN DEMIREL UNIVERSITY   (Turkey)

Author keywords

Accretion, accretion discs; Stars: neutron; X rays: binaries; X rays: individual: 4U 1907+09

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; PULSARS; X RAY ANALYSIS;

ACCRETION: ACCRETION DISKS; HYDROGEN COLUMN DENSITY; PULSE TIMING; SPECTRAL PARAMETERS; SPIN-DOWN; STARS: NEUTRONS; X RAYS: INDIVIDUAL: 4U 1907+09; X-RAY FLUX; X-RAY PULSARS; X-RAYS: BINARIES;

HYDROGEN;

EID: 33745570123     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10412.x     Document Type: Article

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