ISOTHERMAL BLAST WAVE MODEL OF SUPERNOVA-REMNANTS

被引：88

作者：

SOLINGER, A

RAPPAPORT, S

BUFF, J

机构：

[1] MIT,CTR SPACE RES,ROOM 37-411,CAMBRIDGE,MA 02139

[2] MIT,PHYS DEPT,CAMBRIDGE,MA 02139

来源：

ASTROPHYSICAL JOURNAL | 1975年 / 201卷 / 02期

关键词：

D O I：

10.1086/153896

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：381 / 386

页数：6

共 13 条

[1] X-RAY-SPECTRA OF VELA AND PUPPIS SUPERNOVA-REMNANTS AND SHOCK-WAVE MODEL OF SUPERNOVA-REMNANTS [J].

GORENSTEIN, P ;

HARNDEN, FR ;

TUCKER, WH .

ASTROPHYSICAL JOURNAL, 1974, 192 (03) :661-676

[2] SUPERNOVA SHELLS + GALACTIC X-RAYS [J].

HEILES, C .

ASTROPHYSICAL JOURNAL, 1964, 140 (02) :470-&

[3]

HUNDHAUSEN AJ, 1972, CORONAL EXPANSION SO, P77

[4]

KOROBEINIKOV VP, 1956, DOKL AKAD NAUK SSSR+, V109, P271

[5] X-RAY STRUCTURE OF CYGNUS LOOP [J].

RAPPAPORT, S ;

DOXSEY, R ;

SOLINGER, A ;

BORKEN, R .

ASTROPHYSICAL JOURNAL, 1974, 194 (02) :329-+

[6]

Sedov L. I., 1959, SIMILARITY DIMENSION

[7]

SPITZER L, 1962, PHYSICS FULLY IONIZE

[8] THE FORMATION OF A BLAST WAVE BY A VERY INTENSE EXPLOSION .2. THE ATOMIC EXPLOSION OF 1945 [J].

TAYLOR, G .

PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1950, 201 (1065) :175-&

[9] THE FORMATION OF A BLAST WAVE BY A VERY INTENSE EXPLOSION .1. THEORETICAL DISCUSSION [J].

TAYLOR, G .

PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1950, 201 (1065) :159-174

[10]

VASYLIUNAS V, 1975, COMMUNICATION

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