most citedHigh-precision abundances of elements in solar-type stars. Evidence of two distinct sequences in abundance-age relations

124 citations · 145 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2020124 cited

High-precision abundances of elements in solar-type stars. Evidence of two distinct sequences in abundance-age relations

P. E. Nissen, J. Christensen-Dalsgaard, J. R. Mosumgaard +3

HARPS spectra with signal-to-noise ratios S/N > 600 at 6000 A were analysed with MARCS model atmospheres to obtain 1D LTE abundances of C, O, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni, Sr…

astro-ph.GA2020

On the connection between galactic downsizing and the most fundamental galactic scaling relations

E. Spitoni, F. Calura, M. Mignoli +3

In their evolution, star-forming galaxies are known to follow scaling relations between some fundamental physical quantities, such as the mass-metallicity and the main sequence rel…

astro-ph.GA2020

Galactic Archaeology with asteroseismic ages. II. Confirmation of a delayed gas infall using Bayesian analysis based on MCMC methods

E. Spitoni, K. Verma, V. Silva Aguirre +1

With the wealth of information from large surveys and observational campaigns in the contemporary era, it is critical to properly exploit the data to constrain the parameters of Ga…

astro-ph.SR201821 cited

Systematic Differences in Spectroscopic Analysis of Red Giants

Ditte Slumstrup, Frank Grundahl, Victor Silva Aguirre +1

A spectroscopic analysis of stellar spectra can be carried out using different approaches; different methods, line lists, atomic parameters, solar abundances etc. The resulting atm…

astro-ph.GA2018

2D chemical evolution model: the impact of galactic disc asymmetries on azimuthal chemical abundance variations

E. Spitoni, G. Cescutti, I. Minchev +5

Galactic disc chemical evolution models generally ignore azimuthal surface density variation that can introduce chemical abundance azimuthal gradients. Recent observations, however…