Time evolution of abundances of some notable metal-bearing species in the hot cores. — astro-ph.GA Metal-bearing species in diffuse or molecular clouds are often overlooked in astrochemical modeling except for

RGZ EMU user interface and its 3-step workflow setup. The first 2 steps (in blue color) of the workflow is compulsary, while the third (in green color) is optional. —

EWs for the K i lines in the J band vs. NIR spectral type for M dwarfs in our sample. The figure elements are the same as in Figure 3.

Multi-layered pipeline for identifying bacterium/archaeon pairs with similar genomic signatures. Layer 1: Five selected non-parametric clustering methods identify clusters of organisms with similar genomic signatures. The clusters containing both bacteria