Far-infrared spectral studies from the G. P. Kuiper Airborne Observatory

Details Far-infrared spectral studies from the G. P. Kuiper Airborne Observatory Far-infrared spectral studies from the G. P. Kuiper Airborne Observatory

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986cuni.rept.....h&link_type=abstract

Final Technical Report, 1 Oct. 1978 - 31 Oct. 1986 Cornell Univ., Ithaca, NY. Center for Radiophysics and Space Research.

Astronomy and Astrophysics

Astronomy

Far Infrared Radiation, Infrared Astronomy, Spectrum Analysis, Astronomical Observatories, Hydrogen Clouds, Line Spectra, Star Formation, Stellar Evolution

Scientific paper

The grant to carry out far-infrared spectral studies of astronomical sources from the G. P. Kuiper Airborne Observatory was first funded in October 1978 and officially ended on October 31, 1986. During these eight years, A variety of previously undetected spectral lines was discovered, and these were used to determine the physical and chemical conditions prevailing in regions of active star formation. They served to clarify the nature of the ionized hydrogen regions often adjacent to star-forming clouds, the characteristics of shocks which may signify the onset of star formation, and the nature of coolants that channel away energy thus enabling a cloud to collapse to form new stars.

Affiliated with

Also associated with

No associations

Rating

Far-infrared spectral studies from the G. P. Kuiper Airborne Observatory does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Far-infrared spectral studies from the G. P. Kuiper Airborne Observatory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Far-infrared spectral studies from the G. P. Kuiper Airborne Observatory will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1736739