Far-infrared observations of W51 with high spatial resolution

Details Far-infrared observations of W51 with high spatial resolution Far-infrared observations of W51 with high spatial resolution

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196l..31h&link_type=abstract

Astrophysical Journal, vol. 196, Feb. 15, 1975, pt. 2, p. L31-L34.

Astronomy and Astrophysics

Astronomy

36

Far Infrared Radiation, Hydrogen Clouds, Infrared Astronomy, Nebulae, Airborne Equipment, Astronomical Photometry, High Resolution, Interstellar Gas, Jupiter (Planet), Molecular Spectra, Spectral Resolution

Scientific paper

Observations of the core of W51 have been made from the NASA C-141 Airborne Infrared Observatory at 55 microns with 17-, 35-, and 85-arc sec apertures and at 100 microns with a 35-arc sec aperture. These observations suggest the presence of a small less than about 20 arc sec source at 55 microns surrounded by a much broader diffuse background. In the center of the source the optical depth at 55 and 100 microns is on the order of 0.1-0.2.

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