Extrasolar planets: Atmospheres, spectra, and evolution

被引：0
|
作者：
Barman, TS [1 ]
Allard, F [1 ]
Baraffe, I [1 ]
Chabrier, G [1 ]
Hauschildt, PH [1 ]
机构：
[1] Wichita State Univ, Dept Phys, Wichita, KS 67208 USA
来源：
PROCEEDINGS OF THE 13TH CAMBRIDGE WORKSHOP ON COOL STARS, STELLAR SYSTEMS AND THE SUN - PROCEEDINGS, VOLS 1 AND 2 | 2005年 / 560卷
关键词：
planets; exoplanets;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
With the development of new observatories and instruments, the prospects of obtaining direct images and spectroscopy of extrasolar giant planets (EGPs) axe steadily improving. An increasing number of transiting planets are also being discovered which provide more robust tests for EGP evolution models. In this work, models axe presented for the atmospheres, spectra, and evolution of EGPs for a variety of orbital separations and parent star spectral types.
引用
收藏
页码：437 / 440
页数：4
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