Astronomers have conducted high-resolution spectroscopic observations of IRAS 18379-1707 (or LS 5112), a candidate post-asymptotic giant branch (post-AGB) star in the Milky Way galaxy. Results of the observations provide more details about the properties of this object, revealing that it is a metal-poor, high-velocity star. The findings are detailed in a paper published November 28 on arXiv.org.
Astronomers have conducted high-resolution spectroscopic observations of IRAS 18379-1707 (or LS 5112), a candidate post-asymptotic giant branch (post-AGB) star in the Milky Way galaxy. Results of the observations provide more details about the properties of this object, revealing that it is a metal-poor, high-velocity star. The findings are detailed in a paper published November 28 on arXiv.org.
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