INFLUENCE OF ATOMIC DATA ON NON-LTE CHROMOSPHERIC MODELLING

Q4 Physics and Astronomy Astronomical and Astrophysical Transactions Pub Date : 1997-08-01 DOI:10.1080/10556799708213564
S. A. Villegas, R. F. Ferrero
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引用次数: 0

Abstract

Abstract The influence of various kinds of atomic parameters on computed Mg II h and k line profiles is studied. For this purpose, we have run a non-LTE code on several versions of a Mg II model atom differing from one another in the quality and source of the atomic data employed, while keeping fixed the underlying atmospheric structure. With this simple setup we show that employing good quality atomic data is a necessary condition to obtain reliable atmosphere diagnostics. This is of interest in many fields of stellar astrophysics, e. g. semi-empirical chromospheric modelling in our case, but also when modelling external velocity fields, circumstellar/interstellar absorption, etc. and so these data deserve special attention.
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原子数据对非lte色球模型的影响
摘要研究了不同原子参数对计算出的Mg、h、k线轮廓的影响。为此,我们在几个版本的Mg II模型原子上运行了一个非lte代码,这些版本在所用原子数据的质量和来源上彼此不同,同时保持了底层大气结构的固定。通过这种简单的设置,我们表明采用高质量的原子数据是获得可靠的大气诊断的必要条件。这在恒星天体物理学的许多领域都是有意义的,例如在我们的例子中是半经验色球模型,但也在模拟外部速度场,星周/星际吸收等时,因此这些数据值得特别注意。
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来源期刊
Astronomical and Astrophysical Transactions
Astronomical and Astrophysical Transactions Physics and Astronomy-Instrumentation
CiteScore
0.40
自引率
0.00%
发文量
16
期刊介绍: Astronomical and Astrophysical Transactions (AApTr) journal is being published jointly by the Euro-Asian Astronomical Society and Cambridge Scientific Publishers, The journal provides a forum for the rapid publication of material from all modern and classical fields of astronomy and astrophysics, as well as material concerned with astronomical instrumentation and related fundamental sciences. It includes both theoretical and experimental original research papers, short communications, review papers and conference reports.
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