Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.270..329n&link_type=abstract
In ESA, Proceedings of the 8th ESA Symposium on European Rocket and Balloon Programs and Related Research p 329-332 (SEE N88-162
Astronomy and Astrophysics
Astronomy
Balloon-Borne Instruments, Far Infrared Radiation, Infrared Astronomy, Interstellar Space, Line Spectra, Galaxies, Infrared Spectrometers, Interstellar Chemistry, Star Formation
Scientific paper
In the far-infrared part of the spectrum a number of atomic and ionic emission lines occur, which are useful for a study of the physics and chemistry of the interstellar medium and star-forming regions. The present and future situation regarding possibilities of observing these lines is discussed. In particular, the potentials with a small-sized balloon experiment, carrying a cryogenic spectrometer with a large field-of-view (>10 arc minutes) is addressed. Examples are given of galactic and extragalactic objects, which will be observed in the 157.7 μm [C+] emission line.
Nordh Lennart H.
Olofsson S. G.
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