THE EFFECT OF A CIRCUMSTELLAR MEDIUM ON THE X-RAY-EMISSION OF YOUNG REMNANTS OF TYPE-II SUPERNOVAE

被引：73

作者：

ITOH, H ^{[1
]}

MASAI, K ^{[1
]}

机构：

[1] NAGOYA UNIV,INST PLASMA PHYS,CHIKUSA KU,NAGOYA 46401,JAPAN

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1989年 / 236卷 / 04期

关键词：

D O I：

10.1093/mnras/236.4.885

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：885 / 899

页数：15

共 50 条

[1] THE EFFECT OF A CIRCUMSTELLAR MEDIUM ON THE EVOLUTION OF YOUNG REMNANTS OF TYPE-II SUPERNOVAE
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[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1984, 208 (03) : 645 - 659
[2] EMISSION FROM CIRCUMSTELLAR INTERACTION IN NORMAL TYPE-II SUPERNOVAE
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[3] THE HARD X-RAY-EMISSION OF THE YOUNG SUPERNOVA-REMNANTS
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[J]. REPORTS ON PROGRESS IN PHYSICS, 1995, 58 (11) : 1375 - 1413
[8] X-ray emission caused by circumstellar interaction in supernovae
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[J]. FROM TWILIGHT TO HIGHLIGHT: THE PHYSICS OF SUPERNOVAE, 2003, : 315 - 320
[9] STUDIES OF X-RAY-EMISSION FROM SUPERNOVA-REMNANTS
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[J]. PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1974, 340 (1623) : 423 - 437
[10] X-RAY-EMISSION FROM AN INWARD-PROPAGATING SHOCK IN YOUNG SUPERNOVA-REMNANTS
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