activity
20162018
most citedThe IMF as a function of supersonic turbulence

34 citations · 61 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2018

The Gaia-ESO Survey: Evidence of atomic diffusion in M67?

C. Bertelli Motta, A. Pasquali, J. Richer +37

Investigating the chemical homogeneity of stars born from the same molecular cloud at virtually the same time is very important for our understanding of the chemical enrichment of…

astro-ph.SR2017

New massive members of Cygnus OB2

S. R. Berlanas, A. Herrero, F. Comerón +3

The Cygnus complex is one of the most powerful star forming regions at a close distance from the Sun (~1.4 kpc). Its richest OB association Cygnus OB2 is known to harbor many tens…

astro-ph.SR2017

Chemo-Dynamical Clustering applied to APOGEE data: Re-Discovering Globular Clusters

Boquan Chen, Elena D'Onghia, Stephen A. Pardy +4

We have developed a novel technique based on a clustering algorithm which searches for kinematically- and chemically-clustered stars in the APOGEE DR12 Cannon data. As compared to…

astro-ph.SR2017★ 27 cited

Observing the products of stellar evolution in the old open cluster M67 with APOGEE

Clio Bertelli Motta, Maurizio Salaris, Anna Pasquali +1

Recent works have shown how the [C/N] ratio in stars after the first dredge-up (FDU) can be used as an age estimator in virtue of its dependence on stellar mass. For this purpose,…

astro-ph.GA2016★ 34 cited

The IMF as a function of supersonic turbulence

Clio Bertelli Motta, Paul C. Clark, Simon C. O. Glover +2

Recent studies seem to suggest that the stellar initial mass function (IMF) in early-type galaxies might be different from a classical Kroupa or Chabrier IMF, i.e. contain a larger…