The Galactic centre G+0.633-0.0604 molecular cloud: A new astrochemical gold mine: I. Gas physical properties
Departamento de Física de la Tierra y Astrofísica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, Madrid, Spain · Centro de Astrobiología · Centro de Astrobiología · Center for Astrochemical Studies, Max-Planck-Institute für extraterrestrische Physik, Garching bei München, Germany · Joint ALMA Observatory, Vitacura, Santiago, Chile · Centro de Astrobiología · Star and Planet Formation Laboratory, Pioneering Research Institute
astro-ph.GA, astro-ph.SR
Submitted: 2026-07-01
Updated: 2026-09-17
Comments: 20 pages, 11 figures, 8 tables, 6 appendix - Accepted for publication in Astronomy & Astrophysics
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
Related papers
- Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
- Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
- Constraining reionization-era Ly alpha escape with JELS-MUSE: a highly complete H alpha-selected sample at z about6.1
- Deriving volume density profiles of filaments from observed surface densities
- Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
- MEGATRON: how the first stars can create an iron metallicity plateau in the smallest dwarf galaxies