Polarization and kinematic studies of SS 433 indicate a continuous and decelerating jet

Monthly Notices of the Royal Astronomical Society

Volumn 354, Issue 4, 2004, Pages 1239-1254

  Stirling, A M ^a,b   Spencer, R E ^a   Cawthorne, T V ^b   Paragi, Z ^c,d  

^a UNIVERSITY OF MANCHESTER   (United Kingdom)

^b UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^c JOINT INSTITUTE FOR VLBI IN EUROPE   (Netherlands)

^d Foldmeresi es Taverzekelesi Intezet Budapest   (Hungary)

Author keywords

ISM: jets and outflows; Radio continuum: stars; Stars: individual: SS 433

Indexed keywords

ELECTRIC FIELDS; IONIZATION OF GASES; KINEMATICS; MAGNETIC FIELDS; STARS;

CONSTANT VELOCITIES; EJECTION VELOCITY; ISM JETS AND OUTFLOWS; KINEMATICS MODELS; MODEL PREDICTION; PLASMA TUBES; RADIO CONTINUUM: STARS; RADIO IMAGES; STAR: INDIVIDUAL: SS 433; STARS: INDIVIDUAL: PROXIMA CENTAURI;

DEPOLARIZATION;

EID: 8744264009     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08285.x     Document Type: Article

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