activity
20012008
most citedBasic physical parameters of a selected sample of evolved stars

492 citations · 1.3k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph2008★ 2 cited

Testing planet formation theories with Giant stars

Luca Pasquini, M. P. Doellinger, A. Hatzes +4

Planet searches around evolved giant stars are bringing new insights to planet formation theories by virtue of the broader stellar mass range of the host stars compared to the sola…

astro-ph2007★ 171 cited

Evolved stars hint to an external origin of enhanced metallicity in planet-hosting stars

L. Pasquini, M. P. Doellinger, A. Weiss +5

Exo-planets are preferentially found around high metallicity main sequence stars. We aim at investigating whether evolved stars share this property, and what this tells about plane…

astro-ph2007★ 31 cited

Planets around active stars

J. Setiawan, P. Weise, Th. Henning +8

We present the results of radial velocity measurements of two samples of active stars. The first sample contains field G and K giants across the Red Giant Branch, whereas the secon…

astro-ph2007

Physical parameters of evolved stars in clusters and in the field from line-depth ratios

K. Biazzo, L. Pasquini, A. Frasca +6

We present a high-resolution spectroscopic analysis of two samples of evolved stars selected in the field and in the intermediate-age open cluster IC 4651, for which detailed measu…

astro-ph2007★ 52 cited

Abundance analysis of barium and mild barium stars

R. Smiljanic, G. F. Porto de Mello, L. da Silva

High signal to noise, high resolution spectra were obtained for a sample of normal, mild barium, and barium giants. Atmospheric parameters were determined from the FeI and FeII lin…

astro-ph2007★ 22 cited

Deriving temperature, mass and age of evolved stars from high-resolution spectra. Application to field stars and the open cluster IC 4651

K. Biazzo, L. Pasquini, L. Girardi +6

We test our capability of deriving stellar physical parameters of giant stars by analysing a sample of field stars and the well studied open cluster IC 4651 with different spectros…