Submillimeter astronomy and cosmology

Details Submillimeter astronomy and cosmology Submillimeter astronomy and cosmology

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..387...31b&link_type=abstract

Space technology and applications international forum (STAIF - 97). AIP Conference Proceedings, Volume 387, pp. 31-36 (1997).

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Origin And Formation Of The Universe, Observational Cosmology, Star Formation

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In this paper I summarize some key astrophysics questions and the future space missions needed to address them. These missions, and the questions that drive them, fall under the aegis of two of the four thematic areas of NASA's Office of Space Science: ``The Astronomical Search for Origins and Planetary Systems'' covers astrophysics in the near-infrared, optical, and ultraviolet wavelengths (100 μm-912 Å) and ``Structure and Evolution of the Universe,'' covers astrophysics in the remaining gamma-ray, x-ray, far-infrared/submillimeter, and radio wavelengths. This paper focuses on future space missions in the long wavelength (λ>100 μm) regime of the Structure and Evolution of the Universe area.

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