Motif d'Images de la Saint-Patrick avec la Forme et la Rotation Comme Attributs (A)

In the ideal MHD ap- proximation, those are the incompressible Alfv´ en modes (thereafter indexed with A) as well as the fast and slow magnetosonic modes (indexed by F and S), while

Abundances of 11 chemical elements have been determined for 10 F and 12 A dwarfs (“normal” and chemically peculiar) bona-fide and probable members of the Ursa Major Group (age about

Fig. 1 Schematic view of the approach taken to estimate the number CAZyme combinations in PULs. The depolymerization of a given complex glycan by Bacteroidetes PULs requires

However, the inner radius of the circumbinary ring surrounding GG Tau A, measured from both NIR and millimetric observa- tions is dynamically incompatible with the fit of the orbit

We have detected a cloud of neutral and partially ionized gas with a velocity of −15 km s −1 and a hydrogen column density of log N(HI + HII) ∼ 19.3 cm −2 that is thought to

All the models of Procyon A that we computed satisfying the observational constraints of Table 1 have mean large frequency spacing from 53 to 56.5 µHz, compatible with the range of

The high spatial and temporal resolution of the floats data and the biomass and community gradients observed here allow us to study the relationship between mixed layer

size but also slightly on the refractive index, is around 1.94. Figure 7c shows the low values obtained for the SSA express- ing the strong absorbing capability of these aerosols.