ISO Observations of Classical Novae

被引：0
|
作者：
A. Salama
P. Barr
J. Clavel
R. N. Jenkins
K. Leech
M.F. Kessler
T. Lim
L. Metcalfe
B. Schulz
A. Evans
S. P. S. Eyres
机构：
[1] ISO Science Operations Centre,Astrophysics Division, Space Science Department of ESA Villafranca
[2] Keele University,Physics Department
来源：
Astrophysics and Space Science | 1997年 / 255卷 / 1-2期
关键词：
Dust; Physical Condition; Fine Structure; Structure Line; Classical Nova;
D O I：
10.1023/A:1001150716412
中图分类号：
学科分类号：
摘要：
We describe the ISO programme to observe classical novae. The programme includes observations of novae during and shortly after eruption, and old novae. ISO observations of far infrared fine structure lines are providing us with information about physical conditions in nova ejecta which complement and extend knowledge obtained from ground-based observations. Surprisingly, we are getting little information about dust in nova systems, despite the fact that many novae are prolific dust-producers.
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页码：227 / 235
页数：8
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