论文标题

围绕未发展的星星的环和弧形-III。缪斯揭示的行星星云IC 4406中类似环形结构的物理条件

Rings and arcs around evolved stars -- III. Physical conditions of the ring-like structures in the planetary nebula IC 4406 revealed by MUSE

论文作者

Ramos-Larios, G., Toalá, J. A., Rodríguez-González, J. B., Guerrero, M. A., Gómez-González, V. M. A.

论文摘要

We present the analysis of Very Large Telescope (VLT) Multi Unit Spectroscopic Explorer (MUSE) observations of the planetary nebula (PN) IC 4406. MUSE images in key emission lines are used to unveil the presence of at least 5 ring-like structures North and South of the main nebula of IC 4406. MUSE spectra are extracted from the rings to unambiguously assess for the first time in a PN their physical条件,电子密度(NE)和温度(TE)。发现环的TE比主星云的边缘相似,但NE较小。不同离子物种之间的比率表明IC 4406的环的电离状态低于主腔,与猫的眼中NGC6543中建议的环相比。

We present the analysis of Very Large Telescope (VLT) Multi Unit Spectroscopic Explorer (MUSE) observations of the planetary nebula (PN) IC 4406. MUSE images in key emission lines are used to unveil the presence of at least 5 ring-like structures North and South of the main nebula of IC 4406. MUSE spectra are extracted from the rings to unambiguously assess for the first time in a PN their physical conditions, electron density (ne) and temperature (Te). The rings are found to have similar Te than the rim of the main nebula, but smaller ne. Ratios between different ionic species suggest that the rings of IC 4406 have a lower ionization state than the main cavity, in contrast to what was suggested for the rings in NGC6543, the Cat's Eye Nebula.

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