Structure of molecular clouds and space-based sub-millimeter telescopes, for example FIRST

Details Structure of molecular clouds and space-based sub-millimeter telescopes, for example FIRST Structure of molecular clouds and space-based sub-millimeter telescopes, for example FIRST

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.260..295n&link_type=abstract

In ESA Proceedings of an ESA Workshop on a Spaceborne Submillimeter Astronomy Mission. A Cornerstone of the ESA Long Term Scienc

Astronomy and Astrophysics

Astronomy

Astronomical Satellites, Esa Satellites, Infrared Telescopes, Molecular Clouds, Radio Telescopes, Spaceborne Telescopes, Submillimeter Waves, Cloud Physics, Herbig-Haro Objects, Masers, Spaceborne Astronomy, Spatial Distribution, Stellar Envelopes, Stellar Evolution

Scientific paper

Aspects of molecular cloud physics and their associated star forming regions that could be very significantly elucidated by a spaceborne mission such as the ESA Far Infrared Submillimeter Wave Space Telescope (FIRST) are discussed. These include the distribution in external galaxies, cloud substructure, circumstellar disks, bipolar flows, masers, Herbig-Haro objects, and molecular clouds in the Galactic Center. It is emphasized that the highest possible spatial and/or spectral resolution and wavelength coverage are necessary to actually observationally solve these questions and that FIRST has this capability.

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