activity
20082026
most citedThe Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. I. Overview of the Project and Detection of Multiple Stellar Populations

509 citations · 4.3k across the 106 of their papers we have counts for

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Showing 2020Show all

5 papers · 1 filter

astro-ph.GA2020★ 38 cited

Multiple stellar populations along the red Horizontal Branch and Red Clump of Globular Clusters

Emanuele Dondoglio, Antonino P. Milone, Edoardo P. Lagioia +5

We exploit multi-band Hubble Space Telescope photometry to investigate multiple populations (MPs) along the red horizontal branches (HBs) and red clumps of fourteen metal-rich Glob…

astro-ph.GA2020★ 44 cited

The COMBS Survey -- II. Distinguishing the Metal-Poor Bulge from the Halo Interlopers

Madeline Lucey, Keith Hawkins, Melissa Ness +9

The metal-poor stars in the bulge are important relics of the Milky Way's formation history, as simulations predict that they are some of the oldest stars in the Galaxy. In order t…

astro-ph.SR2020★ 17 cited

A chromosome map to unveil stellar populations with different magnesium abundances. The case of Omega Centauri

A. P. Milone, A. F. Marino, A. Renzini +7

Historically, photometry has been largely used to identify stellar populations (MPs) in Globular Clusters (GCs) by using diagrams that are based on colours and magnitudes that are…

astro-ph.SR2020★ 9 cited

The closest extremely low-mass white dwarf to the Sun

Adela Kawka, Jeffrey D. Simpson, Stephane Vennes +4

We present the orbit and properties of 2MASS J050051.85-093054.9, establishing it as the closest (d ~ 71 pc) extremely low mass white dwarf to the Sun. We find that this star is hy…

astro-ph.GA2020★ 29 cited

The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of single and multiple stellar populations in seven bulge globular clusters

R. A. P. Oliveira, S. O. Souza, L. O. Kerber +23

In the present work we analyzed seven globular clusters selected from their location in the Galactic bulge and with metallicity values in the range $-1.30\lesssim\rm{[Fe/H]}\lesssi…