Evidence for a pulsar jet producing a hot nebula in the supernova remnant MSH 15-52

Publications of the Astronomical Society of Japan

Volumn 48, Issue 3, 1996, Pages

  Tamura, Keisuke ^a   Kawai, Nobuyuki ^a   Yoshida, Atsumasa ^a   Brinkmann, Wolfgang ^b  

^a INST OF PHYS AND CHEMICAL RESEARCH   (Japan)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Astrophysical jets; Pulsars; Supernovae, supernova remnants; X rays: Sources

Indexed keywords

HOT ELECTRONS; PULSARS; SUPERNOVAE;

ASTROPHYSICAL JETS; ENERGY; HIGH-ENERGY RESOLUTION; IMAGING CAPABILITIES; RADIO PULSARS; SUPERNOVA REMNANTS; SUPERNOVA, SUPERNOVA REMNANT; X-RAY ASTRONOMY SATELLITES; X-RAY PULSARS; X-RAY SOURCES;

BUDGET CONTROL;

EID: 0030528505     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/48.3.l33     Document Type: Article

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