Calendrier mensuel 2019

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

By comparing the values of the derivatives which are mea- sured by the balloon gradiometer and the same derivatives which are estimated with the use of formulae (11)–(13) from