Analysis of extinction curves towards the SCO OBI association

Mathematics

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Auriga Constellation, Cosmic Dust, Interstellar Extinction, Scorpius Constellation, Goodness Of Fit, Interstellar Matter, Iue, Mathematical Models, Particle Size Distribution, Ultraviolet Radiation

Scientific paper

The UV extinction curves of stars in SCO OBI were analyzed, using different dust models. The first model uses a continuous size distribution; in the second one, single radii for each kind of particle are considered. In both cases, spherical, inorganic, bare particles are considered. The possibility of discriminating among various size distributions was considered. Neither model adequately matches the curves in the whole wavelength range.

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