hot molecular core G10.47+0.03 Archives

Integrated emission maps of detected transitions of CH2NH towards the G10.47+0.03, which are overlaid with the 2.34 mm continuum emission map. The contour levels are 20%, 40%, 60%, and 80% of peak flux. The cyan circle represents the synthesized beam of the integrated emission maps. -- astro-ph.GA

Astrochemistry, Astronomy & Telescopes, Biochemistry & Organic Chemistry, Biophysics, Biosignatures & Paleobiology, Imaging & Spectroscopy, Interstellar, Status Report

Detection And Prebiotic Chemistry of Possible Glycine Precursor Molecule Methylenimine Towards The Hot Molecular Core G10.47+0.03

by Keith CowingApril 19, 2024April 19, 2024

Amino acids are essential for the synthesis of protein. Amino acids contain both amine (R−NH2) and carboxylic acid (R−COOH) functional groups, which help to understand the possible formation mechanism of […]

hot molecular core G10.47+0.03

Detection And Prebiotic Chemistry of Possible Glycine Precursor Molecule Methylenimine Towards The Hot Molecular Core G10.47+0.03

NASA Establishes Mars Forward Operational Risk and Contamination Evaluation (M-FORCE) Tiger Team to Shape Mars Planetary Protection Protocols

Opportunity to Contribute to NASA DARES Community White Paper on Phototrophic Biosignatures

The Search For Life Elsewhere: Avoiding Hype and Fostering Public Understanding

Panchromatic Spectra of Nearby Low-mass and Sun-like Stars with Directly Imageable Habitable Zones

Alfred: A Flexible, User-Friendly Python Package for Exoplanet Confirmation