Collision-induced absorption coefficients of H2 pairs at temperatures from 60 K to 1000 K
Collision-induced absorption coefficients of H2 pairs at temperatures from 60 K to 1000 K
复制标题
60 K 至 1000 K 温度下 H2 对的碰撞诱导吸收系数
DOI：
10.1051/0004-6361:20020555
复制
发表时间：
2002
影响因子：
6.5
通讯作者：
A. Borysow
中科院分区：
文献类型：
--
作者：
A. Borysow
本文首次给出了400 ~ 1000 K温度范围内H2对碰撞诱导吸收的新数据。它们基于对现有“低”温度数据的仔细插值和扩展，这些数据适合用于行星大气建模。新的数据旨在帮助模拟最冷的光环白色矮星，最冷的M型矮星，L型和T型矮星，以及棕矮星和“热木星”。此外，为了方便未来的用户，已经存在的低温（60 K至400 K）数据以一致和用户友好的表格形式提供。已经存在的1000 K以上的数据与这里提供的新数据形成连续序列。从60 K到7000 K的总数据集和从0 cm-1到17 000 cm-1的频率（每10 cm-1计算）现在位于www.astro.ku.dk/aborysow/programs。
New collision-induced absorption data of H2 pairs at temperatures between 400 K and 1000 K are presented here for the first time. They are based on a careful interpolation and extension of the existing 'low' temperature data, which were suited for use in planetary atmospheric modelling. The new data are aimed to help in modelling the coolest halo white dwarfs, the coolest M dwarfs, the L- and T- type dwarf stars, as well as brown dwarfs and "hot jupiters". In addition, for the convenience of the future users, the already existing low temperature (60 K to 400 K) data are provided, in a consistent and user friendly tabular form. The data above 1000 K, which already existed, form a continuous sequence with the new data presented here. The total data set from 60 K to 7000 K and frequencies from 0 cm 1 to17 000 cm 1 (computed for every 10 cm 1 ) is now located at www.astro.ku.dk/aborysow/programs.