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arXiv · 1909.01364

TYC 8606-2025-1: a mild barium star surrounded by the ejecta of a very late thermal pulse

V. V. Gvaramadze·Yu. V. Pakhomov·A. Y. Kniazev·T. A. Ryabchikova·N. Langer·L. Fossati·E. K. Grebel
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Abstract

We report the discovery of a spiral-like nebula with the Wide-field Infrared Survey Explorer (WISE) and the results of optical spectroscopy of its associated star TYC 8606-2025-1 with the Southern African Large Telescope (SALT). We find that TYC 8606-2025-1 is a G8 III star of $\approx3$ M$_\odot$, showing a carbon depletion by a factor of two and a nitrogen enhancement by a factor of three. We also derived an excess of s-process elements, most strongly for barium, which is a factor of three overabundant, indicating that TYC 8606-2025-1 is a mild barium star. We thereby add a new member to the small group of barium stars with circumstellar nebulae. Our radial velocity measurements indicate that TYC 8606-2025-1 has an unseen binary companion. The advanced evolutionary stage of TYC 8606-2025-1, together with the presence of a circumstellar nebula, implies an initial mass of the companion of also about 3 M$_\odot$. We conclude that the infrared nebula, due to its spiral shape, and because it has no optical counterpart, was ejected by the companion as a consequence of a very late thermal pulse, during about one orbital rotation.

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V. V. Gvaramadze, Yu. V. Pakhomov, A. Y. Kniazev, T. A. Ryabchikova, N. Langer, L. Fossati, E. K. Grebel. 2019-09-03. TYC 8606-2025-1: a mild barium star surrounded by the ejecta of a very late thermal pulse. https://doi.org/10.1093/mnras%2Fstz2484

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