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arXiv 2104.02829astro-ph.SR
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TLUSTY和SYNSPEC用户指南IV:升级版208和54

TLUSTY and SYNSPEC Users's Guide IV: Upgraded Versions 208 and 54

Ivan Hubeny, Carlos Allende Prieto, Yeisson Osorio, Thierry Lanz

摘要:

我们提出了一个简短的说明,新升级的版本的程序TLUSTY,版本208,和SYNSPEC,版本54。TLUSTY用于生成恒星大气或吸积盘模型,SYNSPEC生成详细的合成光谱和/或不透明度表。本文补充了已发布的指南,这些指南详细描述了早期版本的代码TLUSTY 205和SYNSPEC 51。主要的升级包括SYNSPEC中不透明度表的灵活构建,以及它们在使用TLUSTY生成混合模型中的使用,其中重要物种在NLTE中处理,而原子和分子线以及连续体的大部分不透明度在LTE中使用预先计算的不透明度表来考虑。还有一些额外的变化和升级,增加了这些代码的多功能性和灵活性。

英文摘要:

We present a brief description of the newly upgraded versions of the programs TLUSTY, version 208, and SYNSPEC, version 54. TLUSTY is used to generate model stellar atmospheres or accretion disks, and SYNSPEC produces detailed synthetic spectra and/or opacity tables. This paper complements published guides that provide a detailed description of earlier versions of the codes, TLUSTY205, and SYNSPEC51. The main upgrades include the flexible construction of opacity tables in SYNSPEC, and their use in producing hybrid models with TLUSTY}, with important species treated in NLTE, while the bulk of opacity of atomic and molecular lines and continua are considered in LTE using a pre-calculated opacity table. There is also a number of additional changes and upgrades that increase the versatility and flexibility of these codes.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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