The spectrum of HD46223

Abstract

The spectrum of HD46223 was established from the optical to the far UV and normalized by the spectrum of a non reddened star of same spectral type. The resulting spectrum is separated into two components. One is the direct starlight. The second is an additional component of light scattered at small angles. In the optical the spectrum is dominated by direct starlight which decreases exponentially due to the linear extinction. Scattered light begins to be noticeable in the near-UV. The near-UV rise of the scattered light is interrupted in the bump region. The wavelength dependence of the scattered light is established in the far-UV, where scattered light dominates the extinction curve. A 1/lambda^4 dependence is found, proving the presence of grains small compared to UV wavelengths. The mathematic expressions of the different components mentionned above give a good fit to the extinction curve in the direction of the star. On a mathematic standpoint the fit can be completed by a Lorentzien for the 2200Ang. bump region. The physical interpretation of the bump may be more difficult to achieve since the paper shows the possibility that only scattered light is extinguished in the bump region. Consequences for the grain size distribution which is necessary to explain the different aspects of scattering in interstellar clouds, for the value of Rv, and problems raised by this interpretation of the spectrum of HD46223, are considered at the end of this paper.

Accepted for publication in New Astronomy. 17 pages, 4 figures

Cited by in corpus (8)

• Early-type stars in the young open cluster NGC 2244 and in the Mon OB2 association I. The multiplicity of O-type stars
• The standard theory of extinction and the spectrum of stars with very little reddening
• Testing New Ideas Regarding the Nature of Interstellar Extinction
• Scattered starlight contamination in the spectrum of reddened stars
• The 2200 A bump and the UV extinction curve
• The incompatibilities between the standard theory of interstellar extinction and observations
• On the relationship between the continuum of interstellar extinction curves, the 2200 Å bump, and the diffuse interstellar bands
• A review of the properties of the scattered starlight which contaminates the spectrum of reddened stars