2000/12/15 by N. Neininger, Neininger, N.
Engineering · Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #Phase Equilibria and Thermodynamics #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0012348
4 pages, 2 figures, to appear in proceedings of IAU Symposium 205: Galaxies and their Constituents at the Highest Angular Resolutions, Manchester UK, August 2000. To be published by ASP, edited by R. Schilizzi, S. Vogel, F. Paresce, M. Elvis
arxiv created 2000/12/15 · openalex publication_date 2000/12/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
I present a unique data set for the study of molecular gas in galaxies: a complete, high-resolution survey of the CO in M31 and additional local studies. The fully sampled survey has an angular resolution of 23" FWHM and the interferometric data attain the pc-scale with sub-arcsecond resolution. For the first time it is now possible to study large and small scales in conjunction. Thus we are able to derive the global structure and study the links down to the individual cloud complexes and star formation regions.