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20062026
most citedThe GALAH Survey: Scientific Motivation

839 citations · 13.1k across the 261 of their papers we have counts for

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Showing 2011Show all

6 papers · 1 filter

astro-ph.GA2011★ 70 cited

The Na-O anticorrelation in horizontal branch stars. I. NGC 2808

R. G. Gratton, S. Lucatello, E. Carretta +3

Globular clusters have been recognized to host multiple stellar populations. A spectacular example of this is the massive cluster NGC2808, where multiple populations have been foun…

astro-ph.GA2011★ 51 cited

A Stromgren view of the multiple populations in globular clusters

Eugenio Carretta, Angela Bragaglia, Raffaele Gratton +2

We discuss a variety of photometric indices assembled from the uvby Stromgren system. Our aim is to examine the pros and cons of the various indices to find the most suitable one(s…

astro-ph.GA2011★ 33 cited

Chemical enrichment mechanisms in Omega Centauri: clues from neutron-capture elements

Valentina D'Orazi, Raffaele Gratton, Elena Pancino +4

In the complex picture of multiple stellar populations in globular clusters (GCs), a special role is played by NGC 5139 Omega Centauri. At variance with the majority of GCs, Omega…

astro-ph.SR2011★ 173 cited

Multiple stellar populations in the globular cluster NGC 1851

Eugenio Carretta, Sara Lucatello, Raffaele Gratton +2

[Abridged] Detailed chemical tagging of individual stellar populations in the Galactic globular cluster (GC) NGC 1851 is presented. Abundances are derived from FLAMES spectra for t…

astro-ph.GA2011★ 55 cited

Multiple populations in Omega Centauri: a cluster analysis of spectroscopic data

Raffaele Gratton, Christian I. Johnson, Sara Lucatello +2

Omega Cen is composed of several stellar populations. Their history might allow us to reconstruct the evolution of this complex object. We performed a statistical cluster analysis…

astro-ph.SR2011★ 50 cited

The debris disk host star HD 61005: a member of the Argus Association?

S. Desidera, E. Covino, S. Messina +6

HD 61005 is a nearby young solar type star that shows a large infrared excess due to a debris disk. The disk has been recently imaged from ground and space, with indications of sev…