activity
19982023
most citedDead or Alive? Long-term evolution of SN 2015bh (SNhunt275)

84 citations · 476 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2023★ 9 cited

A modern view of galaxies and their stellar populations

Pavel Kroupa

A critical discourse is provided on the current status of the astrophysics of galaxies in view of open fundamental questions on the law of gravitation and the physics-driven variat…

astro-ph.SR2022★ 9 cited

The Gaia-ESO Survey: Probing the lithium abundances in old metal-rich dwarf stars in the Solar vicinity

M. L. L. Dantas, G. Guiglion, R. Smiljanic +14

We test a scenario in which radial migration could affect the Li abundance pattern of dwarf stars in the solar neighbourhood. This may confirm that the Li abundance in these stars…

astro-ph.SR2021★ 43 cited

The Gaia-ESO Survey: Target selection of open cluster stars

A. Bragaglia, E. Alfaro, E. Flaccomio +36

The Gaia-ESO Survey (GES) is a public, high-resolution spectroscopic survey with FLAMES@VLT. GES targeted in particular a large sample of open clusters (OCs) of all ages. The diffe…

astro-ph.SR2018★ 77 cited

TOPoS: IV. Chemical abundances from high-resolution observations of seven EMP stars

P. Bonifacio, E. Caffau, M. Spite +15

Extremely metal-poor stars provide us with indirect information on the first generations of massive stars. The TOPoS survey has been designed to increase the census of these stars…

astro-ph.GA2017★ 45 cited

The Gaia -ESO Survey: Lithium enrichment histories of the Galactic thick and thin disc

Xiaoting. Fu, D. Romano, A. Bragaglia +32

Lithium abundance in most of the warm metal-poor main sequence stars shows a constant plateau (A(Li)~2.2 dex) and then the upper envelope of the lithium vs. metallicity distributio…

astro-ph.GA2017★ 30 cited

The Gaia-ESO Survey: Dynamical models of flattened, rotating globular clusters

Sarah M. R. Jeffreson, Jason L. Sanders, N. W. Evans +12

We present a family of self-consistent axisymmetric rotating globular cluster models which are fitted to spectroscopic data for NGC 362, NGC 1851, NGC 2808, NGC 4372, NGC 5927 and…