The double structure of W3-IRS 5 as determined from high-resolution spatial scans

Details The double structure of W3-IRS 5 as determined from high-resolution spatial scans The double structure of W3-IRS 5 as determined from high-resolution spatial scans

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aj.....87..395n&link_type=abstract

Astronomical Journal, vol. 87, Feb. 1982, p. 395-399. NASA-NSF-supported research.

Astronomy and Astrophysics

Astronomy

17

Astronomical Models, Infrared Astronomy, Molecular Clouds, Protostars, Spatial Resolution, Stellar Luminosity, Binary Stars, Black Body Radiation, Energy Distribution, Goodness Of Fit, High Resolution, Interstellar Gas, Radiant Flux Density, Stellar Evolution, Stellar Structure

Scientific paper

Slit scans over the infrared source W3-IRS 5, from 4.8 to 12.7 microns
are interpreted in terms of two sources of luminosity separated by 0.9
arcsec in declination. The data, as a function of wavelength, show that
the two sources must have remarkably similar properties.

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