Structural Parameters of the Thin Disk Population from Evolved Stars in Solar Neighborhood
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arXiv
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| Autores principales: | , , , |
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| Formato: | Preprint |
| Publicado: |
2025
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| _version_ | 1866917887035310080 |
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| author | Iyisan, S. Bilir, S. Tas, O. Onal Plevne, O. |
| author_facet | Iyisan, S. Bilir, S. Tas, O. Onal Plevne, O. |
| contents | This study investigates the structural parameters of the thin-disk population by analyzing the spatial distribution of evolved stars in the solar neighbourhood. From the $\it Gaia$ Data Release 3 database, about 39.1 million stars within 1 kpc and with relative parallax errors $σ_{\varpi}/\varpi\leq 0.10$ were selected. The photometric data was corrected for extinction using a Galactic dust map. The sample was refined by considering the color-magnitude region $M_{\rm G}\times (G_{\rm BP}-G_{\rm RP})_0$ associated with evolved stars, applying a stricter parallax error limit of $σ_{\varpi}/\varpi\leq 0.02$, and yielding 671,600 stars. The star sample was divided into 36 regions based on their Galactic coordinates, with evolved stars in the absolute magnitude range of $-1< M_{\rm G}~{\rm (mag)}\leq 4$ further split into five one-unit magnitude intervals. This led to 180 subgroups whose space density profiles were modelled using a single-component Galaxy model. The analysis shows that the space densities are in agreement with the literature and that the scale heights vary with $200<H~{\rm (pc)}<600$ interval to their absolute magnitudes. Red clump stars in the solar neighbourhood were also estimated to have a scale height of $295\pm10$ pc. These findings indicate that evolved stars with bright absolute magnitudes originate from the evolution of the early spectral-type stars with short scale height, while fainter ones come from the evolution of the intermediate spectral-type stars with large scale height, suggesting variations in scale height reflect the contribution of Galactic evolution processes. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_04079 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Structural Parameters of the Thin Disk Population from Evolved Stars in Solar Neighborhood Iyisan, S. Bilir, S. Tas, O. Onal Plevne, O. Astrophysics of Galaxies This study investigates the structural parameters of the thin-disk population by analyzing the spatial distribution of evolved stars in the solar neighbourhood. From the $\it Gaia$ Data Release 3 database, about 39.1 million stars within 1 kpc and with relative parallax errors $σ_{\varpi}/\varpi\leq 0.10$ were selected. The photometric data was corrected for extinction using a Galactic dust map. The sample was refined by considering the color-magnitude region $M_{\rm G}\times (G_{\rm BP}-G_{\rm RP})_0$ associated with evolved stars, applying a stricter parallax error limit of $σ_{\varpi}/\varpi\leq 0.02$, and yielding 671,600 stars. The star sample was divided into 36 regions based on their Galactic coordinates, with evolved stars in the absolute magnitude range of $-1< M_{\rm G}~{\rm (mag)}\leq 4$ further split into five one-unit magnitude intervals. This led to 180 subgroups whose space density profiles were modelled using a single-component Galaxy model. The analysis shows that the space densities are in agreement with the literature and that the scale heights vary with $200<H~{\rm (pc)}<600$ interval to their absolute magnitudes. Red clump stars in the solar neighbourhood were also estimated to have a scale height of $295\pm10$ pc. These findings indicate that evolved stars with bright absolute magnitudes originate from the evolution of the early spectral-type stars with short scale height, while fainter ones come from the evolution of the intermediate spectral-type stars with large scale height, suggesting variations in scale height reflect the contribution of Galactic evolution processes. |
| title | Structural Parameters of the Thin Disk Population from Evolved Stars in Solar Neighborhood |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2501.04079 |