CAPOS: the bulge Cluster APOgee Survey IX. Spectroscopic Analysis of the Bulge Globular Cluster Terzan 2
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| Autores principales: | , , , , , , , |
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| Formato: | Preprint |
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2025
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| author | Uribe, Macarena Villanova, Sandro Geisler, Douglas Fernández-Trincado, José G. Muñoz, Cesar Barrera, Nicolás Pino, Thaiz Sepúlveda, Franco |
| author_facet | Uribe, Macarena Villanova, Sandro Geisler, Douglas Fernández-Trincado, José G. Muñoz, Cesar Barrera, Nicolás Pino, Thaiz Sepúlveda, Franco |
| contents | We present the first detailed spectroscopic analysis of the heavily extincted bulge globular cluster Terzan 2 (Ter 2) based on high-resolution near-infrared spectra obtained as part of the CAPOS (the bulge Cluster APOgee Survey) project. CAPOS focuses on surveying clusters within the Galactic Bulge, using the APOGEE-2S spectrograph, part of the SDSS-IV survey, a component of the second generation Apache Point Observatory Galactic Evolution Experiment (APOGEE-2). For the spectral analysis, we use the Brussels Automatic Code for Characterizing High accUracy Spectra (BACCHUS) code which provides line-by-line elemental abundances. We derive abundances for Fe-peak (Fe, Ni), $α$-(O, Mg, Si, Ca, Ti), light-(C, N), odd-Z(Al), and the s-process element (Ce) for four members of the cluster. Our analysis yields a mean metallicity of [Fe/H]= $-$0.84 $\pm$ 0.04, with no evidence for an intrinsic variation. We detect a significant abundance variation only in C and N, indicating the presence of multiple populations. Ter 2 exhibits a typical $α$-enrichment, that follows the trend of Galactic GCs. Additionally, our dynamical analysis reveals that Terzan 2 is a bulge globular cluster with a chaotic orbit that is influenced by the Galactic bar but not trapped by it, displaying both prograde and retrograde motions within the inner bulge region. Overall, the chemical patterns observed in Terzan 2 are in good agreement with those of other CAPOS bulge clusters of similar metallicity. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_02385 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | CAPOS: the bulge Cluster APOgee Survey IX. Spectroscopic Analysis of the Bulge Globular Cluster Terzan 2 Uribe, Macarena Villanova, Sandro Geisler, Douglas Fernández-Trincado, José G. Muñoz, Cesar Barrera, Nicolás Pino, Thaiz Sepúlveda, Franco Astrophysics of Galaxies Solar and Stellar Astrophysics We present the first detailed spectroscopic analysis of the heavily extincted bulge globular cluster Terzan 2 (Ter 2) based on high-resolution near-infrared spectra obtained as part of the CAPOS (the bulge Cluster APOgee Survey) project. CAPOS focuses on surveying clusters within the Galactic Bulge, using the APOGEE-2S spectrograph, part of the SDSS-IV survey, a component of the second generation Apache Point Observatory Galactic Evolution Experiment (APOGEE-2). For the spectral analysis, we use the Brussels Automatic Code for Characterizing High accUracy Spectra (BACCHUS) code which provides line-by-line elemental abundances. We derive abundances for Fe-peak (Fe, Ni), $α$-(O, Mg, Si, Ca, Ti), light-(C, N), odd-Z(Al), and the s-process element (Ce) for four members of the cluster. Our analysis yields a mean metallicity of [Fe/H]= $-$0.84 $\pm$ 0.04, with no evidence for an intrinsic variation. We detect a significant abundance variation only in C and N, indicating the presence of multiple populations. Ter 2 exhibits a typical $α$-enrichment, that follows the trend of Galactic GCs. Additionally, our dynamical analysis reveals that Terzan 2 is a bulge globular cluster with a chaotic orbit that is influenced by the Galactic bar but not trapped by it, displaying both prograde and retrograde motions within the inner bulge region. Overall, the chemical patterns observed in Terzan 2 are in good agreement with those of other CAPOS bulge clusters of similar metallicity. |
| title | CAPOS: the bulge Cluster APOgee Survey IX. Spectroscopic Analysis of the Bulge Globular Cluster Terzan 2 |
| topic | Astrophysics of Galaxies Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2509.02385 |