Mira Ceti-Type变量。原子光谱

IF 1.3 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Astrophysical Bulletin Pub Date : 2023-02-08 DOI:10.1134/S1990341322040071
V. E. Panchuk, V. G. Klochkova
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引用次数: 0

摘要

摘要:本文介绍了在光学和近红外波段的光谱观测结果综述的第一部分。列出了主要的现象学方案和模型。在SAO RAS进行的光谱观测和计算补充了已发表的结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Mira Ceti-Type Variables. Atomic Spectra

Abstract—We present the first part of the survey of the results of spectroscopic observations of mirides in the optical and near infrared ranges. The main phenomenological schemes and models are listed. The published results are supplemented by spectroscopic observations and calculations performed at the SAO RAS.

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来源期刊
Astrophysical Bulletin
Astrophysical Bulletin 地学天文-天文与天体物理
CiteScore
2.00
自引率
33.30%
发文量
31
审稿时长
>12 weeks
期刊介绍: Astrophysical Bulletin is an international peer reviewed journal that publishes the results of original research in various areas of modern astronomy and astrophysics, including observational and theoretical astrophysics, physics of the Sun, radio astronomy, stellar astronomy, extragalactic astronomy, cosmology, and astronomy methods and instrumentation.
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