English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
Add to Basket
 Local TagsRelease HistoryDetailsSummary
  The search for multiple populations in Magellanic Clouds clusters - V. Correlation between cluster age and abundance spreads

Martocchia, S., Dalessandro, E., Lardo, C., Cabrera-Ziri, I., Bastian, N., Kozhurina-Platais, V., et al. (2019). The search for multiple populations in Magellanic Clouds clusters - V. Correlation between cluster age and abundance spreads. Monthly Notices of the Royal Astronomical Society, 487, 5324-5334.

Item is

 

show all hide all

Basic

show hide
Item Permalink: https://hdl.handle.net/21.11116/0000-0005-D072-F Version Permalink: https://hdl.handle.net/21.11116/0000-0005-D073-E
Genre: Journal Article

Files

show Files

Locators

show
hide
Locator:
https://ui.adsabs.harvard.edu/abs/2019MNRAS.487.5324M (Any fulltext)
Description:
-
OA-Status:

Creators

show
hide
 Creators:
Martocchia, S.1, Author
Dalessandro, E.1, Author
Lardo, C.1, Author
Cabrera-Ziri, I.1, Author
Bastian, N.1, Author
Kozhurina-Platais, V.1, Author
Salaris, M.1, Author
Chantereau, W.1, Author
Geisler, D.1, Author
Hilker, M.1, Author
Kacharov, N.1, Author
Larsen, S.1, Author
Mucciarelli, A.1, Author
Niederhofer, F.1, Author
Platais, I.1, Author
Usher, C.1, Author
Affiliations:
1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

Content

show
hide
Free keywords: techniques: photometric galaxies: individual: LMC and SMC stars: abundances Astrophysics - Solar and Stellar Astrophysics Astrophysics - Astrophysics of Galaxies
 Abstract: In our HST photometric survey, we have been searching for multiple stellar populations (MPs) in Magellanic Clouds (MCs) massive star clusters which span a significant range of ages (̃1.5-11 Gyr). In the previous papers of the series, we have shown that the age of the cluster represents one of the key factors in shaping the origin of the chemical anomalies. Here, we present the analysis of four additional clusters in the MCs, namely Lindsay 38, Lindsay 113, NGC 2121, and NGC 2155, for which we recently obtained new UV HST observations. These clusters are more massive than ̃104 M☉ and have ages between ̃2.5 and ̃6 Gyr, i.e. located in a previously unexplored region of the cluster age/mass diagram. We found chemical anomalies, in the form of N spreads, in three out of four clusters in the sample, namely in NGC 2121, NGC 2155, and Lindsay 113. By combining data from our survey and HST photometry for three additional clusters in the Milky Way (namely 47 Tuc, M15, and NGC 2419), we show that the extent of the MPs in the form of N spread is a strong function of age, with older clusters having larger N spreads with respect to the younger ones. Hence, we confirm that cluster age plays a significant role in the onset of MPs.

Details

show
hide
Language(s):
 Dates: 2019
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: -
 Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show
hide
Title: Monthly Notices of the Royal Astronomical Society
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: -
Pages: - Volume / Issue: 487 Sequence Number: - Start / End Page: 5324 - 5334 Identifier: -