| Full text | |
| Author(s): Show less - |
Fabiano de Souza, G.
;
Estera, P. W.
;
Almeida-Fernandes, F. .
;
Limberg, G.
;
Dias, B.
;
Hernandez-Jimenez, J. A.
;
Herpich, F. R.
;
Kerber, L. O.
;
Machado-Pereira, E.
;
Perottoni, H. D.
;
Guerco, Rafael
;
Li, L.
;
Sampedro, L.
;
Kanaan, A.
;
Ribeiro, T.
;
Schoenell, W.
;
Mendes de Oliveira, C.
Total Authors: 17
|
| Document type: | Journal article |
| Source: | Monthly Notices of the Royal Astronomical Society; v. 527, n. 2, p. 12-pg., 2024-01-01. |
| Abstract | |
The Magellanic Clouds are the most massive and closest satellite galaxies of the Milky Way (MW), with stars covering ages from a few Myr up to 13 Gyr. This makes them important for validating integrated light methods to study stellar populations and star formation processes, which can be applied to more distant galaxies. We characterized a set of stellar clusters in the Small Magellanic Cloud (SMC), using the Southern Photometric Local Universe Survey. This is the first age (metallicity) determination for 11 (65) clusters of this sample. Through its seven narrow bands, centred on important spectral features, and five broad bands, we can retrieve detailed information about stellar populations. We obtained ages and metallicities for all stellar clusters using the Bayesian spectral energy distribution fitting code BAGPIPES. With a sample of clusters in the colour range -0.20 < r - z < +0.35, for which our determined parameters are most reliable, we modeled the age-metallicity relation of SMC. At any given age, the metallicities of SMC clusters are lower than those of both the Gaia Sausage-Enceladus disrupted dwarf galaxy and the MW. In comparison with literature values, differences are log(age) 0.31 and Fe/H] 0.41, which is comparable to low-resolution spectroscopy of individual stars. Finally, we confirm a previously known gradient, with younger clusters in the centre and older ones preferentially located in the outermost regions. On the other hand, we found no evidence of a significant metallicity gradient. (AU) | |
| FAPESP's process: | 21/09468-1 - Study of stellar populations in the S-PLUS survey |
| Grantee: | Felipe de Almeida Fernandes |
| Support Opportunities: | Scholarships abroad - Research Internship - Post-doctor |
| FAPESP's process: | 21/10429-0 - The chemodynamical structure of the ancient galactic halo |
| Grantee: | Guilherme Limberg |
| Support Opportunities: | Scholarships in Brazil - Doctorate (Direct) |
| FAPESP's process: | 18/20977-2 - Identification of giant stars for mapping our Galaxy in the S-PLUS survey |
| Grantee: | Felipe de Almeida Fernandes |
| Support Opportunities: | Scholarships in Brazil - Post-Doctoral |