| タイトル | Community Plan for Far-Infrared/Submillimeter Space Astronomy |
| 本文（外部サイト） | http://hdl.handle.net/2060/20040074304 |
| 著者（英） | Ali, Shafinaz; Benford, Dominic; Borne, Kirk; Amato, Michael; Blain, Andrew; Baker, Charles; Ade, Peter; Arendt, Richard; Bock, James; Akeson, Rachel |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2004-04-01 |
| 言語 | eng |
| 内容記述 | This paper represents the consensus view of the 124 participants in the Second Workshop on New Concepts for Far-Infrared/Submillimeter Space Astronomy.We recommend that NASA pursue the vision for far-IR astronomy outlined in the NAS Decadal Survey, which said: A rational coordinated program for space optical and infrared astronomy would build on the experience gained with NGST1 to construct [a JWST-scale filled-aperture far-IR telescope SAFIR, and then ultimately, in the decade 2010 to 2020, build on the SAFIR, TPF, and SIM experience to assemble a space-based, far-infrared interferometer. SAFIR will study star formation in the young universe, the buildup of elements heavier than hydrogen over cosmic history, the process of galaxy formation, and the early phases of star formation, which occur behind a veil of dust that precludes detection at mid IR and shorter wavelengths. The far-infrared interferometer will resolve distant galaxies to study protogalaxy interactions and mergers and the processes that led to enhanced star formation activity and the formation of Active Galactic Nuclei, and will resolve protostars and debris disks in our Galaxy to study how stars and planetary systems form. |
| NASA分類 | Astronomy |
| 権利 | No Copyright |
|
