2004/12/16 by C. L. Carilli, Carilli, C. L.
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0412437
esapub.cls, 8 pages, 10 figures. to appear in: "Dusty04 -- A prelude to Herschel and ALMA" ESA Publication SP-577, ed. A. Wilson & F. Combes
arxiv created 2004/12/16 · openalex publication_date 2004/12/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
With the ability to see into optically obscured regions with more than an order of magnitude better sensitivity and spatial resolution relative to current (sub)mm telescopes, ALMA will provide a unique look into the physics of galaxy formation and active galactic nuclei. In this paper I summarize the ALMA potential for studying star forming galaxies and active galactic nuclei from the nearby universe to the epoch of formation of the first luminous objects.