Chengyuan Li
THE VMC SURVEY. XI. RADIAL STELLAR POPULATION GRADIENTS IN THE GALACTIC GLOBULAR CLUSTER 47 TUCANAE
Li, Chengyuan; de Grijs, Richard; Deng, Licai; Rubele, Stefano; Wang, Chuchu; Bekki, Kenji; Cioni, Maria-Rosa L.; Clementini, Gisella; Emerson, Jim; For, Bi-Qing; Girardi, Leo; Groenewegen, Martin A. T.; Guandalini, Roald; Gullieuszik, Marco; Marconi, Marcella; Piatti, Andrés E.; Ripepi, Vincenzo; van Loon, Jacco Th.
Authors
Richard de Grijs
Licai Deng
Stefano Rubele
Chuchu Wang
Kenji Bekki
Maria-Rosa L. Cioni
Gisella Clementini
Jim Emerson
Bi-Qing For
Leo Girardi
Martin A. T. Groenewegen
Roald Guandalini
Marco Gullieuszik
Marcella Marconi
Andrés E. Piatti
Vincenzo Ripepi
Jacobus Van Loon j.t.van.loon@keele.ac.uk
Abstract
We present a deep near-infrared color–magnitude diagram of the Galactic globular cluster 47 Tucanae, obtained with the Visible and Infrared Survey Telescope for Astronomy (VISTA) as part of the VISTA near-infrared Y, J, Ks survey of the Magellanic System (VMC). The cluster stars comprising both the subgiant and red giant branches exhibit apparent, continuous variations in color–magnitude space as a function of radius. Subgiant branch stars at larger radii are systematically brighter than their counterparts closer to the cluster core; similarly, red-giant-branch stars in the cluster's periphery are bluer than their more centrally located cousins. The observations can very well be described by adopting an age spread of ∼0.5 Gyr as well as radial gradients in both the cluster's helium abundance (Y) and metallicity (Z), which change gradually from (Y = 0.28, Z = 0.005) in the cluster core to (Y = 0.25, Z = 0.003) in its periphery. We conclude that the cluster's inner regions host a significant fraction of second-generation stars, which decreases with increasing radius; the stellar population in the 47 Tuc periphery is well approximated by a simple stellar population.
Citation
Li, C., de Grijs, R., Deng, L., Rubele, S., Wang, C., Bekki, K., Cioni, M.-R. L., Clementini, G., Emerson, J., For, B.-Q., Girardi, L., Groenewegen, M. A. T., Guandalini, R., Gullieuszik, M., Marconi, M., Piatti, A. E., Ripepi, V., & van Loon, J. T. (in press). THE VMC SURVEY. XI. RADIAL STELLAR POPULATION GRADIENTS IN THE GALACTIC GLOBULAR CLUSTER 47 TUCANAE. Astrophysical Journal, 790(1), 35. https://doi.org/10.1088/0004-637x/790/1/35
Journal Article Type | Article |
---|---|
Acceptance Date | May 28, 2014 |
Online Publication Date | Jun 30, 2014 |
Deposit Date | Jun 16, 2023 |
Journal | The Astrophysical Journal |
Print ISSN | 0004-637X |
Electronic ISSN | 1538-4357 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 790 |
Issue | 1 |
Pages | 35 |
DOI | https://doi.org/10.1088/0004-637x/790/1/35 |
Keywords | Space and Planetary Science; Astronomy and Astrophysics |
Public URL | https://keele-repository.worktribe.com/output/473327 |
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