Archive for November, 202565- Page

D/H ratios for CH2DOH (left panel) and CH3OD (right panel) across the star-forming sequence. The spread per source type was calculated using all column densities listed in Table A. The

Set of iCOMs considered in this work. Color code: red for oxygen, white for hydrogen, gray for carbon, and blue for nitrogen. — The Astrophysical Journal Interstellar dust grains are

Chaperone-assisted protein remodeling enables microbial survival under extreme composting heat. During hyperthermophilic composting, microbial communities endure temperatures approaching 87 °C by activating a network of heat shock proteins that stabilize

Self-consistent obliquity and spin rate evolution for several realizations of exoplanet Kepler-79 d. Trajectories go from right to left. The planet is initalized with a spin rate of 7.5 hours

Left, the free fluids phase and Fe-enriched blebs are entrained in the magma ocean. Center: water is outgassed to create a steam atmosphere while the Fe-enriched blebs sink toward the

WASP-39b 3D model cross sections. Shown are the local gas temperature, Tgas (left) and cloud dust-to-gas mass ratio, ρdust/ρgas (right). The values are derived from the 3D GCM results