A study of (OI) 63.2 and 145.5 micron emission from M17 and SGR A from the Lear jet

Details A study of (OI) 63.2 and 145.5 micron emission from M17 and SGR A from the Lear jet A study of (OI) 63.2 and 145.5 micron emission from M17 and SGR A from the Lear jet

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sao..reptq....m&link_type=abstract

Final Report, 1 Oct. 1982 - 31 Mar. 1986 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Hydrogen, Interstellar Matter, Molecular Clouds, Recombination Reactions, Stellar Luminosity, Carbon, Emission Spectra, H Ii Regions, Lear Jet Aircraft, Line Spectra, Nebulae, Research Aircraft, Telescopes

Scientific paper

The Lear Jet Observatory was used to observe the 157.7 micron (C II) line from the galactic H II regions W3 and W51. These measurements established a lower limit in the 157.7 micron line for solar luminosity of 360 from W3, assuming adistance of 2 kpc, and a solar luminosity of 4100 from W51, assuming a distance of 7 kpc. The data indicated that the CII/far infrared continuum ratio for both W3 and W51 were within the range found for other galactic H II regions.

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