On the origin of the system PSR B 1757-24/SNR G 5.4-1.2

Astronomy and Astrophysics

Volumn 415, Issue 3, 2004, Pages 1073-1078

  Gvaramadze, V V ^a,b,c  

^a MOSCOW STATE UNIVERSITY   (Russian Federation)

^b INSTITUTE OF PHYSICS   (Georgia)

^c ABDUS SALAM INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS   (Italy)

Author keywords

ISM: bubbles ISM: individual objects: G 5.4 1.2; ISM: supernova remnants; Pulsars: individual: PSR B 1757 24

Indexed keywords

MAGNETIC FIELD EFFECTS; MAGNETIZATION; MATHEMATICAL MODELS; OBSERVATORIES; SPACE RESEARCH;

MACH NUMBER; STAR; SUPERNOVA REMNANT; WIND BLOWN BUBBLE;

ASTROPHYSICS;

EID: 1542276538     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034631     Document Type: Article

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