{ "id": "astro-ph/9410023", "version": "v1", "published": "1994-10-06T15:37:51.000Z", "updated": "1994-10-06T15:37:51.000Z", "title": "Dispersal and Mixing of Oxygen in the Interstellar Medium of Gas-Rich Galaxies", "authors": [ "Jean-Rene ROY", "Daniel KUNTH" ], "comment": "Latex file 30 pages, accepted in A&A", "categories": [ "astro-ph" ], "abstract": "Stellar and nebular abundance indicators reveal that there exists significant abundance fluctuations in the interstellar medium (ISM) of gas-rich galaxies. It is shown that at the present observed solar level of O/H $\\sim 6 \\times 10^{-4}$, abundance differences of a factor of two, such as existing between the Sun and the nearby Orion Nebula, are many times larger than expected. We examine a variety of hydrodynamical processes operating at scales ranging from 1 pc to greater than 10 kpc, and show that the ISM should appear better homogenized chemically than it actually is: $(i)$ on large galactic scales (1 $\\geq\\ l\\ \\geq$ 10 kpc), turbulent diffusion of interstellar clouds in the shear flow of galactic differential rotation is able to wipe out azimuthal O/H fluctuations in less than $10^9$ yrs; $(ii)$ at the intermediate scale (100 $\\geq\\ l\\ \\geq$ 1000 pc), cloud collisions and expanding supershells driven by evolving associations of massive stars, differential rotation and triggered star formation will re-distribute and mix gas efficiently in about $10^8$ yrs; $(iii)$ at small scales (1 $\\geq\\ l\\ \\geq$ 100 pc), turbulent diffusion may be the dominant mechanism in cold clouds, while Rayleigh-Taylor and Kelvin-Helmhotz instabilities quickly develop in regions of gas ionized by massive stars, leading to full mixing in", "revisions": [ { "version": "v1", "updated": "1994-10-06T15:37:51.000Z" } ], "analyses": { "keywords": [ "interstellar medium", "gas-rich galaxies", "turbulent diffusion", "nebular abundance indicators reveal", "azimuthal o/h fluctuations" ], "note": { "typesetting": "LaTeX", "pages": 30, "language": "en", "license": "arXiv", "status": "editable", "inspire": 390657 } } }