On the Dependence of our Inferences about the Solar Internal Rotation on the Frequency Fitting Methodology
We show how inferences of the solar internal rotation rate depend on different aspects of the mode fitting procedure. We study the stability of the rotation...
On the Detectability of Post-common-envelope Binary Central Stars of Planetary Nebulae
Common envelope evolution is widely accepted as the principal shaping agent in the formation of aspherical planetary nebulae. However, only some 20% of...
On the Determination of Magnetic Field Strength and Flux in Inter-Network
The results of the determination of magnetic field strength and flux from weak polarimetric signals in solar inter-network regions are contradictory. We...
On the direct determination of sensitivity, resolution and information content of helioseismic data application to the inversion of the solar core rotation rate
On the elusive detection of O-type stars close to the ZAMS: the empirical birthline of massive stars
In this contribution we present the results from a 1 homogeneous quantitative spectroscopic analysis of ∼400 Galactic O-type stars targeted by the IACOB and OWN...
On the evidence of extra mixing in models of 8 M⊙ computed with the new solar abundances
Stars more massive than about 3M⊙ are known to experience loops in the HR diagram during their core helium burning phase. Except for very massive stars the...