Condense
发表于 2025-3-26 23:56:35
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Chromatic
发表于 2025-3-27 02:08:16
NLTE Radiative Transfer in Cool Stars, stellar spectra and element abundances. We also compile and analyse the most recent results from the literature. In particular, we examine the NLTE effects for 24 chemical elements for six well-studied FGK-type stars.
Flounder
发表于 2025-3-27 07:05:34
Spectral Classification: The First Step in Quantitative Spectral Analysis,Classification lies at the foundation of many sciences, and that is true for Astronomy as well. However, many stellar spectroscopists neglect this vital first step when carrying out a spectral analysis. This chapter discusses and illustrates the ways that spectral classification can contribute to spectroscopic analysis at every step of the process.
戏法
发表于 2025-3-27 10:10:55
Determination of Atmospheric Parameters of B-, A-, F- and G-Type StarsLectures from the Sc
可商量
发表于 2025-3-27 17:05:22
2190-5193 at the Wrocław‘s Spectroscopic School aimed at training young researchers in performing quantitative spectral analysis of low-, mid-, and high-resolution spectra of B, A, and F-type stars.978-3-319-38302-6978-3-319-06956-2Series ISSN 2190-5193 Series E-ISSN 2190-5207
原谅
发表于 2025-3-27 19:40:22
Ewa Niemczura,Barry Smalley,Wojtek PychOffers an introduction to the theory of stellar atmospheres.Contains step-by-step tutorials on how to determine basic stellar parameters.Provides an introduction to the 3D and non-LTE analysis of stel
鄙视读作
发表于 2025-3-27 22:55:36
GeoPlanet: Earth and Planetary Scienceshttp://image.papertrans.cn/d/image/269317.jpg
大范围流行
发表于 2025-3-28 02:46:57
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闲荡
发表于 2025-3-28 06:42:05
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Substance
发表于 2025-3-28 13:14:47
Elicitor Recognition and Signal Transductionions. The main sources of atomic parameters are different databases that collect laboratory or theoretical data from original publications. A brief review of spectroscopic databases, that are most important for stellar astrophysics is presented.