activity
20112023
most citedThe Pisa pre-main sequence tracks and isochrones. A database covering a wide range of Z, Y, mass, and age values

285 citations · 1.4k across the 38 of their papers we have counts for

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Showing 2019Show all

5 papers · 1 filter

astro-ph.SR2019★ 7 cited

Evidence of a substellar companion to AB Dor C

J. B. Climent, J. P. Berger, J. C. Guirado +5

Studies of fundamental parameters of very low-mass objects are indispensable to provide tests of stellar evolution models that are used to derive theoretical masses of brown dwarfs…

astro-ph.GA2019★ 64 cited

The Gaia-ESO survey: Calibrating a relationship between Age and the [C/N] abundance ratio with open clusters

G. Casali, L. Magrini, E. Tognelli +51

In the era of large high-resolution spectroscopic surveys, high-quality spectra can contribute to our understanding of the Galactic chemical evolution, providing chemical abundance…

astro-ph.SR2019★ 18 cited

The Gaia-ESO Survey: The inner disc, intermediate-age open cluster Pismis 18

D. Hatzidimitriou, E. V. Held, E. Tognelli +34

Pismis 18 is a moderately populated, intermediate-age open cluster located within the solar circle at a Galactocentric distance of about 7 kpc. Few open clusters have been studied…

astro-ph.SR2019★ 54 cited

When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster

Tereza Jerabkova, Giacomo Beccari, Henri M. J. Boffin +5

The high-quality OmegaCAM photometry of the 3x3 deg around the Orion Nebula Cluster (ONC) in r, and i filters by Beccari et al.(2017) revealed three well-separated pre-main sequenc…

astro-ph.SR2019★ 36 cited

The Gaia-ESO Survey: age spread in the star forming region NGC6530 from the HR diagram and gravity indicators

L. Prisinzano, F. Damiani, V. Kalari +33

In very young clusters, stellar age distribution is the empirical proof of the duration of star formation (SF) and of the physical mechanisms involved in the process. We derived ac…