Phenomenology of pulsar B0809+74's rotating subbeam system: I. Geometry and profile "absorption"

Astronomy and Astrophysics

Volumn 447, Issue 1, 2006, Pages 235-243

  Rankin, Joanna M ^a,e   Ramachandran, R ^b   Suleymanova, Svetlana A ^c,d  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c Pushchino Radio Astronomy Observatory   (Russian Federation)

^d Isaac Newton Institute of Chile   (Russian Federation)

^e University of Vermont   (United States)

Author keywords

Polarisation; Radiation mechanisms: non thermal; Stars: pulsars: individual: B0809+74

Indexed keywords

QUANTITATIVE ESTIMATES; RADIATION MECHANISMS: NON-THERMAL; ROTATING SUBBEAM; STARS: PULSARS: INDIVIDUAL: B0809+74;

GEOMETRY; LIGHT SCATTERING; MECHANISMS; POLARIZATION; RADIATION EFFECTS;

ASTRONOMY;

EID: 32544442377     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20042310     Document Type: Article

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