We report the spectroscopic discovery of abundance spreads (i.e. multiple populations) in the 1/42 Gyr old cluster in the LMC, Hodge 6. We use low-resolution VLT FORS2 spectra of 15 member stars in the cluster to measure their CN and CH band strengths at ' 3883 and 4300 Å, respectively, as well as [C/Fe] and [N/Fe] abundances. We find a subpopulation of two stars that are enriched in nitrogen, and we conclude that this subpopulation is evidence of multiple populations in Hodge 6. This is the second 1/42 Gyr old cluster (the first being NGC 1978 in the LMC) to show multiple populations and the first spectroscopic detection of MPs in a cluster of this age. This result is interesting as it hints at a possible relationship between the disappearance of extended main sequence turn-offs in clusters younger than 1/42 Gyr and the onset of multiple populations at 1/42 Gyr, which should be explored further.
Hollyhead K., Martocchia S., Lardo C., Bastian N., Kacharov N., Niederhofer F., et al. (2019). Spectroscopic detection of multiple populations in the er Hodge 6 in the LMC. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 484(4), 4718-4725 [10.1093/mnras/stz317].
Spectroscopic detection of multiple populations in the er Hodge 6 in the LMC
Lardo C.;Mucciarelli A.;
2019
Abstract
We report the spectroscopic discovery of abundance spreads (i.e. multiple populations) in the 1/42 Gyr old cluster in the LMC, Hodge 6. We use low-resolution VLT FORS2 spectra of 15 member stars in the cluster to measure their CN and CH band strengths at ' 3883 and 4300 Å, respectively, as well as [C/Fe] and [N/Fe] abundances. We find a subpopulation of two stars that are enriched in nitrogen, and we conclude that this subpopulation is evidence of multiple populations in Hodge 6. This is the second 1/42 Gyr old cluster (the first being NGC 1978 in the LMC) to show multiple populations and the first spectroscopic detection of MPs in a cluster of this age. This result is interesting as it hints at a possible relationship between the disappearance of extended main sequence turn-offs in clusters younger than 1/42 Gyr and the onset of multiple populations at 1/42 Gyr, which should be explored further.File | Dimensione | Formato | |
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