Extreme ultraviolet astronomy

被引:48
作者
Bowyer, S [1 ]
Drake, JJ
Vennes, S
机构
[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[3] Australian Natl Univ, Sch Math Sci, Astrophys Theory Ctr, Canberra, ACT 0200, Australia
关键词
planets; interstellar medium; stars; extragalactic;
D O I
10.1146/annurev.astro.38.1.231
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Astronomical studies in the extreme ultraviolet (EW) band of the spectrum were dismissed during the early years of space astronomy as impossible, primarily because of the mistaken view that radiation in this band would be absorbed by the interstellar medium. Observations in the 1980s from sounding rockets and limited duration orbital spacecraft began to show the potential of this field and led to the deployment of two spacecraft devoted to EUV astronomy: the UK Wide Field Camera and the Extreme Ultraviolet Explorer. The instrumentation in these missions, although quite limited in comparison with instrumentation in other fields of space astronomy, provided unique and far-reaching results. These included new information on solar system topics, stellar chromospheres and corona, white dwarf astrophysics, cataclysmic variables, the interstellar medium, galaxies, and clusters of galaxies. We summarize these findings herein.
引用
收藏
页码:231 / 288
页数:58
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