A search for 100 mu m and sub-mm emission in dwarf novae

被引：3
|
作者：
Howell, SB [1 ]
Herzog, A [1 ]
Robson, I [1 ]
机构：
[1] JOINT ASTRON CTR,HILO,HI 96720
来源：
ASTRONOMICAL JOURNAL | 1996年 / 111卷 / 02期
关键词：
D O I：
10.1086/117836
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Harrison & Gerhz [AJ, 103, 243 (1992)] noted that IRAS had apparently detected a few quiescent dwarf novae at 100 mu m. This possible detection was intriguing as dwarf novae were not anticipated to be emitters of such long-wavelength radiation. In order to confirm or place limits on this emission, we have undertaken a reanalysis of the IRAS database for four of their ''100 mu m'' dwarf novae. We have also made preliminary sub-mm radio observations of three additional dwarf novae. We find null detections for all our sources in both the IRAS database and in the sub-mm radio range. (C) 1996 American Astronomical Society.
引用
收藏
页码：899 / 901
页数：3
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