Detection of Low-Level Activities in Solar-Analog Stars from the Emission Strengths of Ca II 3934 Line
Yoichi Takeda, Akito Tajitsu, Satoshi Honda, Satoshi Kawanomoto,, Hiroyasu Ando, and Takashi Sakurai

TL;DR
This study measures low-level chromospheric activity in 118 solar-analog stars using Ca II 3934 line emission, revealing the Sun's activity level and challenging previous ideas about Maunder-minimum stars.
Contribution
It introduces a precise method for detecting subtle chromospheric activities in solar analogs, improving sensitivity down to log R' ~ -5.4, and provides new insights into the Sun's activity status.
Findings
The Sun's activity level is near the low end among solar analogs.
Low-level activities can be reliably detected with the new measurement technique.
The high frequency of Maunder-minimum stars with lower activity is unlikely.
Abstract
Activity studies of solar-type stars, especially with reference to the status of our current Sun among them, have exposed the importance of (1) homogeneously selecting the sample stars and (2) reliably evaluating their activities down to a considerably low level. Motivated by these requirements, we conducted an extensive study on the activities of 118 solar-analog stars (of sufficiently similar properties to each other) by measuring the emission strength at the core of Ca II 3933.663 line (K line) on the high-dispersion spectrogram obtained by Subaru/HDS, where special attention was paid to correctly detecting the chromospheric emission by removing the wing-fitted photospheric profile calculated from the classical solar model atmosphere. This enabled us to detect low-level activities down to log R' ~ -5.4 (R' is the ratio of the chromospheric core emission flux to the total bolometric…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
