Multiple stellar populations in the globular cluster M3 (NGC 5272): a Strömgren perspective
dc.contributor.author | Massari, D. | |
dc.contributor.author | Lapenna, E. | |
dc.contributor.author | Bragaglia, A. | |
dc.contributor.author | Dalessandro, E. | |
dc.contributor.author | Contreras Ramos, Rodrigo Andrés | |
dc.contributor.author | Amigo Fuentes, Pía | |
dc.date.accessioned | 2021-05-13T17:51:30Z | |
dc.date.available | 2021-05-13T17:51:30Z | |
dc.date.issued | 2016 | |
dc.description.abstract | We present Strömgren photometry of the Galactic Globular Cluster M3 to study its multiple generations phenomenon. The use of different colour–magnitude diagrams (CMDs) and especially of the notoriously efficient c y index allowed us to detect a double red giant branch in the cluster CMD. After decontamination from fore- and background sources, the two sequences turned out to be equally populated. The two components also show a bimodal radial distribution well corresponding to that predicted by numerical simulations for clusters living in an intermediate dynamical evolutive state and with a population with modified chemical composition that was born more centrally concentrated than the primordial. The analysis of high-resolution spectra quantitatively demonstrates that the two detected sequences correspond to the first (Na-poor) generation and the second (Na-rich) generation, thus confirming the importance of synergy between photometry and spectroscopy. | |
dc.format.extent | 10 páginas | |
dc.fuente.origen | OUP | |
dc.identifier.doi | 10.1093/mnras/stw583 | |
dc.identifier.eissn | 1365-2966 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.uri | https://ieeexplore.ieee.org/stamp/stamp.jsp?arnumber=8344066 | |
dc.identifier.uri | https://doi.org/10.1093/mnras/stw583 | |
dc.information.autoruc | Instituto de astrofísica ; Contreras Ramos, Rodrigo Andrés ; S/I ; 3820 | |
dc.information.autoruc | Instituto de física ; Amigo Fuentes, Pía. ; S/I ; 131179 | |
dc.issue.numero | 4 | |
dc.language.iso | en | |
dc.nota.acceso | Contenido parcial | |
dc.pagina.final | 4171 | |
dc.pagina.inicio | 4162 | |
dc.publisher | OUP | |
dc.revista | Monthly Notices of the Royal Astronomical Society | es_ES |
dc.revista | Monthly Notices of the Royal Astronomical Society | |
dc.rights | acceso restringido | |
dc.title | Multiple stellar populations in the globular cluster M3 (NGC 5272): a Strömgren perspective | es_ES |
dc.type | artículo | |
dc.volumen | 458 | |
sipa.codpersvinculados | 3820 | |
sipa.codpersvinculados | 131179 |
Files
Original bundle
1 - 1 of 1
Loading...
- Name:
- Multiple stellar populations in the globular cluster M3 (NGC 5272) a Stromgren perspective.pdf
- Size:
- 54.66 KB
- Format:
- Adobe Portable Document Format
- Description: