Spectroscopic properties of the H-3(+) molecule: A new calculated line list

被引：196

作者：

Neale, L ^{[1
]}

Miller, S ^{[1
]}

Tennyson, J ^{[1
]}

机构：

[1] HARVARD SMITHSONIAN CTR ASTROPHYS, INST THEORET ATOM & MOLEC PHYS, CAMBRIDGE, MA 02138 USA

来源：

ASTROPHYSICAL JOURNAL | 1996年 / 464卷 / 01期

关键词：

infrared; general; line; identification; molecular data; planets and satellites; stars; atmospheres;

D O I：

10.1086/177341

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A new list of H-3(+) infrared transition frequencies and intensities is presented. This list greatly extends the range of transitions considered to both higher energy and higher rotational states. The 3 x 10(6) transitions are found to significantly affect both the absorption coefficient of H-3(+) and its cooling properties at temperatures above 1000 K. It is hoped these new data will be used for models of cool stars of low metallicity, the giant planets, and other warm bodies composed largely of H-2.

引用

页码：516 / 520

页数：5

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