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arXiv · 1612.02993

Chromospheric activity on the late-type star V1355 Ori using Lijiang 1.8-m and 2.4-m telescopes

Qing-Feng Pi·Li-Yun Zhang·Liang Chang·Xian-Ming Han·Hong-Peng Lu·Xi-Liang Zhang·Dai-Mei Wang
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Abstract

We obtained new high-resolution spectra using the Lijiang 1.8-m and 2.4-m telescopes to investigate the chromospheric activities of V1355 Ori as indicated in the behaviors of Ca ii H&K, Hdelta, Hgamma, Hbeta, Na i D1, D2, Halpha and Ca ii infrared triplet (IRT) lines. The observed spectra show obvious emissions above the continuum in Ca ii H&K lines, absorptions in the Hdelta, Hgamma, Hbeta and Na i D1, D2 lines, variable behavior (filled-in absorption, partial emission with a core absorption component or emission above the continuum) in the Halpha line, and weak self-reversal emissions in the strong filled-in absorptions of the Ca ii IRT lines. We used a spectral subtraction technique to analyze our data. The results show no excess emission in the Hdelta and Hgamma lines, very weak excess emissions in the Na i D1, D2 lines, excess emission in the Hbeta line, clear excess emission in the Halpha line, and excess emissions in the Ca ii IRT lines. The value of the ratio of EW8542/EW8498 is in the range 0.9 to 1.7, which implies that chromospheric activity might have been caused by plage events. The value of the ratio E Halpha/E Hbeta is above 3, indicating that the Balmer lines would arise from prominence-like material. We also found time variations in light curves associated with equivalent widths of chromospheric activity lines in the Na i D1, D2, Ca ii IRT and Halpha lines in particular. These phenomena can be explained by plage events, which are consistent with the behavior of chromospheric activity indicators.

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Qing-Feng Pi, Li-Yun Zhang, Liang Chang, Xian-Ming Han, Hong-Peng Lu, Xi-Liang Zhang, Dai-Mei Wang. 2016-12-09. Chromospheric activity on the late-type star V1355 Ori using Lijiang 1.8-m and 2.4-m telescopes. https://doi.org/10.1088/1674-4527%2F16%2F10%2F153

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