High-resolution maps of H2 regions at far-infrared wavelengths

Details High-resolution maps of H2 regions at far-infrared wavelengths High-resolution maps of H2 regions at far-infrared wavelengths

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf...79f&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 79-85 (SEE

Physics

Optics

3

Astronomical Maps, Balloon-Borne Instruments, Far Infrared Radiation, High Resolution, Hydrogen Clouds, Cassegrain Optics, Infrared Astronomy, Nebulae, Orion Constellation, Radiation Sources, Telescopes

Scientific paper

The first successful flight of a balloon-borne 1-m telescope for far-infrared (40 micron) astronomy occurred on 4 February 1974 (UT), from Palestine, Texas. During 6 h at float altitude, the gyrostabilized telescope mapped the intensity of far-infrared radiation from the H 2 regions Ori A and W3 with a resolution of 1 prime. Partial maps of these regions were made with a resolution of 0.5 prime. These sources were resolved into several components, some of which were previously unknown. Observations of Mars were used for calibration.

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