Rare Find: Discovery and chemo-dynamical properties of two s-process enhanced RR Lyrae stars
Fuente:
arXiv
Saved in:
| Main Authors: | , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866908675098017792 |
|---|---|
| author | D'Orazi, Valentina Iorio, Giuliano Cseh, Borbála Sneden, Chris Abdollahi, Hedieh Molnár, László Bobrick, Alexey Bono, Giuseppe Braga, Vittorio F. Karakas, Amanda Lugaro, Maria Campbell, Simon W. Fabrizio, Michele Fiorentino, Giuliana Roederer, Ian U. Storm, Nicholas Tantalo, Maria Crestani, Juliana |
| author_facet | D'Orazi, Valentina Iorio, Giuliano Cseh, Borbála Sneden, Chris Abdollahi, Hedieh Molnár, László Bobrick, Alexey Bono, Giuseppe Braga, Vittorio F. Karakas, Amanda Lugaro, Maria Campbell, Simon W. Fabrizio, Michele Fiorentino, Giuliana Roederer, Ian U. Storm, Nicholas Tantalo, Maria Crestani, Juliana |
| contents | We report the serendipitous discovery of two RR Lyrae stars exhibiting significant s-process element enrichment, a rare class previously represented solely by TY Gruis. Our goal is to characterise these objects chemically and dynamically, exploring their origins and evolutionary histories. Using high-resolution spectroscopy from HERMES@AAT and UVES@VLT, we derived detailed chemical abundances of key s-process elements, carbon along with $α$-elements. We also employed Gaia DR3 astrometric data to analyse their kinematics, orbital properties, and classify their Galactic population membership. We compared observational results with theoretical asymptotic giant branch nucleosynthesis models to interpret their enrichment patterns. Both stars exhibit clear signatures of s-process enrichment, with significant overabundances in second-peak elements such as Ba and La compared to first-peak Y and Zr. Comparison with AGB nucleosynthesis models suggests their progenitors experienced pollution of s-process-rich material, consistent with early binary interactions. However, notable discrepancies in dilution factors highlight the need for more refined low-metallicity asymptotic giant branch (AGB) models. We also explore and discuss alternative scenarios, including sub-luminous post-AGB-like evolution or double episodes of mass transfer. Our findings confirm the existence of s-process-enhanced RR Lyrae stars and demonstrate the importance of combining chemical and dynamical diagnostics to unveil their complex evolutionary pathways. Future detailed binary evolution modelling and long-term orbital monitoring are essential to resolve their formation scenarios and assess the role of binarity in the evolution of pulsating variables. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2510_15723 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Rare Find: Discovery and chemo-dynamical properties of two s-process enhanced RR Lyrae stars D'Orazi, Valentina Iorio, Giuliano Cseh, Borbála Sneden, Chris Abdollahi, Hedieh Molnár, László Bobrick, Alexey Bono, Giuseppe Braga, Vittorio F. Karakas, Amanda Lugaro, Maria Campbell, Simon W. Fabrizio, Michele Fiorentino, Giuliana Roederer, Ian U. Storm, Nicholas Tantalo, Maria Crestani, Juliana Solar and Stellar Astrophysics We report the serendipitous discovery of two RR Lyrae stars exhibiting significant s-process element enrichment, a rare class previously represented solely by TY Gruis. Our goal is to characterise these objects chemically and dynamically, exploring their origins and evolutionary histories. Using high-resolution spectroscopy from HERMES@AAT and UVES@VLT, we derived detailed chemical abundances of key s-process elements, carbon along with $α$-elements. We also employed Gaia DR3 astrometric data to analyse their kinematics, orbital properties, and classify their Galactic population membership. We compared observational results with theoretical asymptotic giant branch nucleosynthesis models to interpret their enrichment patterns. Both stars exhibit clear signatures of s-process enrichment, with significant overabundances in second-peak elements such as Ba and La compared to first-peak Y and Zr. Comparison with AGB nucleosynthesis models suggests their progenitors experienced pollution of s-process-rich material, consistent with early binary interactions. However, notable discrepancies in dilution factors highlight the need for more refined low-metallicity asymptotic giant branch (AGB) models. We also explore and discuss alternative scenarios, including sub-luminous post-AGB-like evolution or double episodes of mass transfer. Our findings confirm the existence of s-process-enhanced RR Lyrae stars and demonstrate the importance of combining chemical and dynamical diagnostics to unveil their complex evolutionary pathways. Future detailed binary evolution modelling and long-term orbital monitoring are essential to resolve their formation scenarios and assess the role of binarity in the evolution of pulsating variables. |
| title | Rare Find: Discovery and chemo-dynamical properties of two s-process enhanced RR Lyrae stars |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2510.15723 |