The infrared angular diameter of Eta Carinae

Astronomy and Astrophysics – Astronomy

Scientific paper

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Infrared Astronomy, Novae, Stellar Envelopes, Stellar Luminosity, Diameters, H Lines, Instrument Errors, Normal Density Functions, Spatial Distribution, Stellar Spectrophotometry, Wavelengths

Scientific paper

Infrared observations of the cool shell around Eta Car between 3.7 and 12.2 microns were obtained by a described method which is comparable to iris-photometry of photographic plates. Half-flux diameters, which increase smoothly with wavelength from 2.7 arcsec to 6.5 arcsec, were calculated; circular symmetry and Gaussian intensity distribution are assumed. The importance of deviations from simple Gaussian shape was estimated by performing a deconvolution which applies the sum of the two Gaussians for both the observed and the instrumental response functions. The half-flux diameters calculated by this method were typically 25% lower than the values found by the first method, and reasons for preferring the first set of values are presented.

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