Infrared emission from novae

被引：0
|
作者：
Evans, A. [1 ]
Gehrz, R. D. [2 ]
机构：
[1] Keele Univ, Lennard Jones Lab, Astrophys Grp, Keele ST5 5BG, Staffs, England
[2] Univ Minnesota, Sch Phys & Astron, Minnesota Inst Astrophys, Minneapolis, MN 55455 USA
来源：
BULLETIN OF THE ASTRONOMICAL SOCIETY OF INDIA | 2012年 / 40卷 / 03期
关键词：
classical novae; recurrent novae; infrared observations; circumstellar matter; CASSIOPEIAE; 1993; CLASSICAL NOVAE; RS-OPHIUCHI; SILICATE DUST; TEMPORAL DEVELOPMENT; GRAIN-GROWTH; MASS-LOSS; SPITZER; SPECTROSCOPY; VULPECULAE;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We review infrared observations of classical and recurrent novae, at wavelengths > 3 mu m, including both broad-band and spectroscopic observations. In recent years infrared spectroscopy in particular has revolutionised our understanding of the nova phenomenon, by revealing fine-structure and coronal lines, and the mineralogy of nova dust. Infrared spectroscopic facilities that are, or will be, becoming available in the next 10-20 years have the potential for a comprehensive study of nova line emission and dust mineralogy, and for an unbiased assessment of the extragalactic nova populations.
引用
收藏
页码：213 / 241
页数：29
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