The nature of the PSR J2051-0827 eclipses

Monthly Notices of the Royal Astronomical Society

Volumn 321, Issue 3, 2001, Pages 576-584

  Stappers, B W ^a   Bailes, M ^b   Lyne, A G ^c   Camilo, F ^d   Manchester, R N ^e   Sandhu, J S ^f   Toscano, M ^c,g   Bell, J F ^e  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^c UNIVERSITY OF MANCHESTER   (United Kingdom)

^d Och Spine at New York Presbyterian Hospitals   (United States)

^e CSIRO   (Australia)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g UNIVERSITY OF MELBOURNE   (Australia)

Author keywords

Binaries: eclipsing; PSR J2051 0827; Pulsars: individual; Stars: neutron

Indexed keywords

MAGNETOSPHERE;

BINARIES:ECLIPSING; FLUX DENSITIES; HIGH FREQUENCY HF; LOWER FREQUENCIES; PSR J2051-0827; PULSARS:INDIVIDUAL; PULSE TIME; STARS: NEUTRONS; TIMES OF ARRIVALS; WIDE FREQUENCY RANGE;

PULSARS;

EID: 0040947241     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04074.x     Document Type: Article

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