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Table · dataset · 2010

Effective temperatures of Ap stars

Listed in IVOA Registry (Virtual Observatory)

A new method of determination of the effective temperatures of Ap stars is proposed.

Description

The method is based on the fact that the slopes of the energy distribution in the Balmer continuum near the Balmer jump for "normal" main sequence stars and Ap stars with the same effective temperature are identical. The effective temperature calibration is based on a sample of main sequence stars with well known temperatures (Sokolov, 1995, Cat. <J/A+AS/110/553>).

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