CO EMISSION FROM SUPERNOVA-REMNANTS

被引：76

作者：

SCOVILLE, NZ ^{[1
]}

IRVINE, WM ^{[1
]}

WANNIER, PG ^{[1
]}

PREDMORE, CR ^{[1
]}

机构：

[1] UNIV MASSACHUSETTS,DEPT PHYS & ASTRON,AMHERST,MA 01003

来源：

ASTROPHYSICAL JOURNAL | 1977年 / 216卷 / 01期

关键词：

D O I：

10.1086/155473

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：320 / 328

页数：9

共 46 条

[1] EXPANDING SHELL OF NEUTRAL HYDROGEN SURROUNDING SUPERNOVA REMNANT HB-21 [J].

ASSOUSA, GE ;

ERKES, JW .

ASTRONOMICAL JOURNAL, 1973, 78 (09) :885-893

[2]

BYCHKOV KV, 1975, SOVIET ASTRONOMY LET, V1, P29

[3]

CHEVALIER RA, 1974, ASTROPHYS J, V188, P501, DOI 10.1086/152740

[4] EVOLUTION OF SUPERNOVA-REMNANTS .4. SUPERNOVA EJECTA [J].

CHEVALIER, RA .

ASTROPHYSICAL JOURNAL, 1975, 200 (03) :698-708

[5] SOME IMPLICATIONS OF X-RAY DATA FROM OLD SUPERNOVA-REMNANTS [J].

CLARK, DH ;

CULHANE, JL .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1976, 175 (03) :573-586

[6] OBSERVATIONS OF CYGNUS LOOP AT 408-MHZ [J].

COLLA, G ;

MARANO, B ;

GANDOLFI, E ;

LARI, C ;

FANTI, C ;

FANTI, R ;

FORMIGGINI, L ;

EICARRA, A ;

TOMASI, P ;

SALTER, CJ ;

SETTI, G ;

PADRIELL, L .

ASTRONOMICAL JOURNAL, 1971, 76 (10) :956-+

[7] HYDRODYNAMIC INSTABILITIES AND FORMATION OF RADIO SHELLS IN YOUNG SUPERNOVAE REMNANTS [J].

COWIE, LL .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1975, 173 (02) :429-436

[8] EVOLUTIONARY THERMAL MODEL FOR CYGNUS LOOP [J].

COX, DP .

ASTROPHYSICAL JOURNAL, 1972, 178 (01) :169-&

[9] IONIZATION EQUILIBRIUM AND RADIATIVE COOLING OF A LOW-DENSITY PLASMA [J].

COX, DP ;

TUCKER, WH .

ASTROPHYSICAL JOURNAL, 1969, 157 (3P1) :1157-&

[10] PHYSICAL CONDITIONS IN INTERSTELLAR HYDROXYL AND FORMALDEHYDE CLOUDS [J].

DAVIES, RD ;

MATTHEWS, HE .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1972, 156 (02) :253-&

← 1 2 3 4 5 →