Pulsar microstructure and its quasi-periodicities with the S2 VLBI system at a resolution of 62.5 nanoseconds

Astronomy and Astrophysics

Volumn 396, Issue 1, 2002, Pages 171-187

  Popov, M V ^a   Bartel, N ^b   Cannon, W H ^b   Novikov, A Yu ^b   Kondratiev, V I ^a   Altunin, V I ^c  

^a LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

^b YORK UNIVERSITY   (Canada)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Methods: data analysis; Methods: observational; Radio continuum: stars; Stars: pulsars: general

Indexed keywords

DATA REDUCTION; MAGNETIC FIELD EFFECTS; MAGNETOSPHERE; MICROSTRUCTURE; NEUTRON EMISSION; SIGNAL PROCESSING;

PULSAR RADIO EMISSIONS;

ASTROPHYSICS;

EID: 0036898081     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021402     Document Type: Article

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