Application of the infrared flux method to 3 cool AP stars (78 Virginis, 52 HerculisA and CS Virginis) and comparison of their energy distributions to model atmospheres

Astronomy and Astrophysics – Astronomy

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A Stars, Cool Stars, Infrared Astronomy, Peculiar Stars, Spectral Energy Distribution, Stellar Atmospheres, Metallicity, Stellar Models, Stellar Rotation, Stellar Temperature

Scientific paper

The infrared flux method proposed by Blackwell and Shallis (1977) is used, along with a comparison of the observed energy distribution to model grids, in order to determine the fundamental parameters of three cool Ap stars: 78 Vir, 52HerA, and CS Vir. The degree to which their energy distributions can be reproduced using currently available model atmospheres is shown.

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