RADIO SUPERNOVAE

被引：274

作者：

WEILER, KW

SRAMEK, RA

PANAGIA, N

VANDERHULST, JM

SALVATI, M

机构：

[1] USN,RES LAB,NATL SCI FDN,WASHINGTON,DC 20375

[2] SPACE TELESCOPE SCI INST,BALTIMORE,MD 21218

[3] CNR,IST ASTROFIS SPAZIALE,I-00044 FRASCATI,ITALY

[4] CNR,IST RADIOASTRON,ROME,ITALY

[5] NETHERLANDS FDN RADIO ASTRON,DWINGELOO,NETHERLANDS

来源：

ASTROPHYSICAL JOURNAL | 1986年 / 301卷 / 02期

关键词：

D O I：

10.1086/163944

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：790 / 812

页数：23

共 104 条

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[2]

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[4]

ARGYLE RW, 1984, IAU3985 CIRC

[5]

ARGYLE RW, 1984, IAU3912 CIRC

[6] TYPE-I SUPER-NOVAE .1. ANALYTIC SOLUTIONS FOR THE EARLY PART OF THE LIGHT-CURVE [J].

ARNETT, WD .

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[7]

BANDIERA R, 1983, ASTRON ASTROPHYS, V126, P7

[8] THE EVOLUTION OF NONTHERMAL SUPERNOVA-REMNANTS .2. CAN RADIO SUPERNOVAE BECOME PLERIONS [J].

BANDIERA, R ;

PACINI, F ;

SALVATI, M .

ASTROPHYSICAL JOURNAL, 1984, 285 (01) :134-140

[9]

BARBON R, 1982, ASTRON ASTROPHYS, V116, P35

[10]

Barbon R., 1984, Astronomy & Astrophysics Supplement Series, V58, P735

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