CONSEQUENCES OF A NEW HOT COMPONENT OF INTERSTELLAR-MEDIUM

被引：731

作者：

SHAPIRO, PR

FIELD, GB

机构：

[1] HARVARD-SMITHSONIAN ASTROPHYS OBSERV,CTR ASTROPHYS,CAMBRIDGE,MA 02138

[2] HARVARD-SMITHSONIAN ASTROPHYS OBSERV,CAMBRIDGE,MA 02138

来源：

ASTROPHYSICAL JOURNAL | 1976年 / 205卷 / 03期

关键词：

D O I：

10.1086/154332

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：762 / 765

页数：4

共 21 条

[1]

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[4]

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[5] LARGE-SCALE EFFECTS OF SUPERNOVA-REMNANTS ON GALAXY - GENERATION AND MAINTENANCE OF A HOT NETWORK OF TUNNELS [J].

COX, DP ;

SMITH, BW .

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[6]

FIELD GB, 268 CTR ASTR PREPR

[7]

FIELD GB, 1975, 1974 LES HOUCH SUMM

[8] APERTURE SYNTHESIS OF INTERSTELLAR NEUTRAL HYDROGEN IN ABSORPTION .2. CYGNUS A, CRAB-NEBULA, AND OTHER SOURCES [J].

GREISEN, EW .

ASTROPHYSICAL JOURNAL, 1973, 184 (02) :379-396

[9] APERTURE SYNTHESIS OF INTERSTELLAR NEUTRAL HYDROGEN IN ABSORPTION .1. PERSEUS ARM FEATURE OF CASSIOPEIA A [J].

GREISEN, EW .

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[10]

HEILES C, 1974, GALACTIC RADIO ASTRO, P13

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