HYACINTH Archives

Column density maps of different species in the simulated galaxy after post-processing. The total hydrogen and H2 from the simulation are shown in the first two panels. The remaining panels show the column density of H2, C+ , C, and CO obtained via post-processing. The H2 from post-processing (top row, third panel) is remarkably similar to the H2 from the simulation (top row, second panel). CO dominates the carbon budget in the highest NH2 regions and is essentially absent when NH2 ≲ 1021 cm−2 . Atomic carbon traces the full extent of the H2 distribution while C + extends farther out to regions devoid of a significant amount of H2 -- astro-ph.GA

AI - Data - Apps - Cybernetics, Astrochemistry, Imaging & Spectroscopy, Interstellar, Status Report

HYACINTH: HYdrogen And Carbon chemistry In The INTerstellar Medium In Hydro Simulations

by Keith CowingFebruary 21, 2024February 20, 2024

Aims. We present a new sub-grid model, HYACINTH — HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations, for computing the non-equilibrium abundances of H2 and its carbon-based […]

HYACINTH

HYACINTH: HYdrogen And Carbon chemistry In The INTerstellar Medium In Hydro Simulations

Determining The “Biosignature Threshold” For Life Detection On Biotic, Abiotic, or Prebiotic Worlds.

Icy Ocean Planet Research: NASA ROSES-25 Amendment 71: New Opportunity A.16 Cryosphere

Global Carbon Fixation In Earth’s Subsurface Biosphere

tinyRNA-seq: An Optimized Approach To Sequencing Tiny RNAs And Primitive RNA Genomes

Stellar Flares Rather Than High Tint As Possible Cause For the Missing Methane In Young Exoplanets: The Case Study of V1298-Tau b