Multi-wavelength spectral energey distributions and determination of effective temperatures using the infrared flux method for A and F dwarfs

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The spectral energy distributions (SEDs) from the UV to IR have been constructed for 83 main sequence A and F stars for which ultraviolet (IUE), optical spectrophotometries and IR photometry are available. Their effective temperature were derived using the Infrared Flux Method ( IRFM ). Finally, the constructed SEDs have been compared to the predictions of ATLAS12 for the found IRFM temperatures, adequate surface gravities and chemical composition when available to test the ability of models to reproduce the SEDs.

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