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Titolo:
INTERACTION OF JETS WITH A SUPERNOVA REMNANT IN THE SS 433 W50 SYSTEM/
Autore:
MURATA K; SHIBAZAKI N;
Indirizzi:
RIKKYO UNIV,DEPT PHYS,TOSHIMA KU TOKYO 171 JAPAN
Titolo Testata:
Publications of the Astronomical Society of Japan
fascicolo: 6, volume: 48, anno: 1996,
pagine: 819 - 825
SICI:
0004-6264(1996)48:6<819:IOJWAS>2.0.ZU;2-I
Fonte:
ISI
Lingua:
ENG
Soggetto:
SS-433; PULSAR; ACCELERATION; MODELS; NEBULA; SS433; SHOCK;
Keywords:
ASTROPHYSICAL JETS; RADIATION MECHANISMS; SHOCK WAVES; STARS, INDIVIDUAL (SS 433); SUPERNOVA REMNANTS, INDIVIDUAL (W50);
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Science Citation Index Expanded
Citazioni:
21
Recensione:
Indirizzi per estratti:
Citazione:
K. Murata e N. Shibazaki, "INTERACTION OF JETS WITH A SUPERNOVA REMNANT IN THE SS 433 W50 SYSTEM/", Publications of the Astronomical Society of Japan, 48(6), 1996, pp. 819-825

Abstract

The well known for the precessing relativistic jet SS 433 is located near to the center of the radio source W50. The radio shell of W50 is elongated in the direction of the jets to give ear-like structures. X-ray lobes are found between the radio ears and SS 433. We consider theinteraction of the jets with the supernova remnant shell for the radio ears and X-ray lobes. We show that the expansion of the shell is enhanced at the part which in being pushed by the jets to yield the ear-like structures, and that the electrons accelerated at the reverse shocks emit synchrotron X-rays; as observed from the lobes. Comparing withthe observations, we set constraints on the physical properties of the jets and interstellar matter.

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Documento generato il 04/12/20 alle ore 16:32:10