Calendrier Mensuel 2002 (A)

that, (i) objects with photometry compatible with the cluster se- quence but in the proper motions halo, have higher membership probabilities in our methodology due to the

In order to determine the validity of the previous dielectric mixing model, we performed complex permittivity measurements for a sand/sea water mixture with the

Using a Monte Carlo uncertainty method to compute the theo- retical error of molecular abundances in chemical models, we found a strong sensitivity of the steady-state abundances to

isotope ratios derived from absorption lines from diffuse or translucent clouds (Sgr B2(N)) are consistent with values derived from emission lines from a prominent star-forming

The method was first devised using TGAS data in CG18, and successfully applied to a low-density disc region (the Galactic anticentre) using Gaia DR2 in CG19, finding a total of 76

We invert global black carbon (BC), organic car- bon (OC) and desert dust (DD) aerosol emissions from POLDER/PARASOL spectral aerosol optical depth (AOD) and aerosol absorption

This work analyzed the intermittency and the scaling prop- erties of the wind speed v ant the aggregate power out- put P time series, through structure function analysis, at all

Consequently, comparing the results for the FULL model with the UP- SCAL model for which particles are forced to exit the immobile domain where they entered for each of the