IRAS OBSERVATIONS OF SUPERNOVA-REMNANTS - A COMPARISON BETWEEN THEIR INFRARED AND X-RAY COOLING RATES

被引:47
作者
DWEK, E
PETRE, R
SZYMKOWIAK, A
RICE, WL
机构
[1] NASA,GODDARD SPACE FLIGHT CTR,HIGH ENERGY ASTROPHYS LAB,GREENBELT,MD 20771
[2] CALTECH,JET PROP LAB,PASADENA,CA 91109
关键词
D O I
10.1086/184971
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:L27 / L33
页数:7
相关论文
共 41 条
[1]  
ARENDT RG, 1987, COMMUNICATION
[2]  
BRAUN R, 1986, ASTRON ASTROPHYS, V164, P208
[3]  
BRAUN R, 1986, ASTRON ASTROPHYS, V164, P193
[4]  
BRAUN R, 1987, ASTRON ASTROPHYS, V171, P233
[5]  
BRAUN R, 1987, COMMUNICATION
[6]   DUST GRAINS IN A HOT GAS .1. BASIC PHYSICS [J].
BURKE, JR ;
SILK, J .
ASTROPHYSICAL JOURNAL, 1974, 190 (01) :1-10
[7]   COLLING AND EVOLUTION OF A SUPERNOVA REMNANT [J].
COX, DP .
ASTROPHYSICAL JOURNAL, 1972, 178 (01) :159-+
[8]   HEATING AND IONIZATION OF HI REGIONS [J].
DALGARNO, A ;
MCCRAY, RA .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1972, 10 :375-+
[9]  
DINERSTEIN HL, 1986, AP J, V312, P314
[10]   INFRARED-EMISSION FROM DUST IN SHOCKED GAS [J].
DRAINE, BT .
ASTROPHYSICAL JOURNAL, 1981, 245 (03) :880-890