Recent submillimetre wavelength studies of molecules in star formation regions

Details Recent submillimetre wavelength studies of molecules in star formation regions Recent submillimetre wavelength studies of molecules in star formation regions

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.189....5w&link_type=abstract

In ESA The Sci. Importance of Submillimetre Observations p 5-11 (SEE N83-22034 11-88)

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2

Atmospheric Attenuation, High Altitude, Interstellar Matter, Line Spectra, Molecular Clouds, Radiation Trapping, Water Vapor, Density (Mass/Volume), Hydrogen, Instrument Compensation, Michelson Interferometers, Radio Telescopes, Spectroscopy

Scientific paper

The recent availability of sensitive heterodyne detectors in the submillimetre spectral region (300-1000 GHz) and large aperture optical infrared telescopes at high altitude observatories have led to sensitive astronomical observations of a number of molecular species in galactic star formation regions. The current state of progress in this newly developing field is examined both with regard to present day detectors and also astrophysical applications.

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