activity
19972016
most citedOn the mass-to-light ratio of the local Galactic disc and the optical luminosity of the Galaxy

350 citations · 768 across the 8 of their papers we have counts for

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22 papers · 1 filter

astro-ph2007★ 119 cited

The Helium abundance and Delta Y / Delta Z in Lower Main Sequence stars

Luca Casagrande, Chris Flynn, Laura Portinari +2

We use nearby K dwarf stars to measure the helium-to-metal enrichment ratio, a diagnostic of the chemical history of the Solar Neighbourhood. Our sample of K dwarfs has homogeneous…

astro-ph2006★ 195 cited

Accurate fundamental parameters for Lower Main Sequence Stars

L. Casagrande, L. Portinari, C. Flynn

We derive an empirical effective temperature and bolometric luminosity calibration for G and K dwarfs, by applying our own implementation of the InfraRed Flux Method to multi-band…

astro-ph2006★ 350 cited

On the mass-to-light ratio of the local Galactic disc and the optical luminosity of the Galaxy

Chris Flynn, Johan Holmberg, Laura Portinari +2

We measure the volume luminosity density and surface luminosity density generated by the Galactic disc, using accurate data on the local luminosity function and the disc's vertical…

astro-ph2006★ 44 cited

The Tully-Fisher relation and its evolution with redshift in cosmological simulations of disc galaxy formation

Laura Portinari, Jesper Sommer-Larsen

We present predictions on the evolution of the Tully-Fisher (TF) relation with redshift, based on cosmological N-body/hydrodynamical simulations of disc galaxy formation and evolut…

astro-ph2005

The colours of the Sun

Johan Holmberg, Chris Flynn, Laura Portinari

We compile a sample of Sun-like stars with accurate effective temperatures, metallicities and colours (from the UV to the near-IR). A crucial improvement is that the effective temp…

astro-ph2005

Simulating galaxy clusters -- I. Thermal and chemical properties of the intra-cluster medium

A. D. Romeo, J. Sommer-Larsen, L. Portinari +1

We have performed a series of N-body/hydrodynamical (TreeSPH) simulations of clusters and groups of galaxies, selected from cosmological N-body simulations within a CDM framewor…