Pollux: A weak dynamo-driven dipolar magnetic field and implications for its probable planet

Figure 3(D) shows the change in the extinction coefficient as a function of time with the OISI total hemoglobin change ΔHBT and the OCT flow in a vein [labeled in Fig.. Both the

Leurs résultats confirment que la déshydratation est à l'origine de la perte de résistance à la corrosion observée après un vieillissement à température

Ces expressions se sont transformées, dans le langage actuel, en « avoir ou tenir quelqu’un à l’œil » ; « ne dormir que d’un œil », traduisant le fait de ne pas

Accompanying data are palynological preparation and slide numbers (all prefixed by MCP and NMW 2017) followed by England Finder coordinates.. For authors, see

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We therefore propose the hypothesis that stars on the two branches have distinct magnetic field topologies - dominantly poloidal fields on the inactive branch while active branch

With an inclination i = 40 ◦ , which is the most prob- able value obtained when the star’s rotation and the planet’s orbital motion are assumed to be tidally locked, the

We investigate the extent to which the weak vs strong field bistability predicted for the geodynamo can apply to recent observations of two groups of very low mass