Discovery of the high-field polar RXJ1724.0+4114

We report the discovery of a new AM Herculis binary (polar) as the optical counterpart of the soft X-ray source RXJ1724.0+4114 detected during the ROSAT all-sky survey. The magnetic nature of this V ∼ 17m object is confirmed by low-resolution spectroscopy showing strong Balmer and HeII emission lines superimposed on a blue continuum which is deeply modulated by cyclotron humps. The inferred magnetic field strength is 50±4 MG (or possibly even ≈ 70 MG). Photometric observations spanning ∼ 3 years reveal a period of 119.9 min, right below the period gap. The morphology of the optical and X-ray light curves which do not show eclipses by the secondary star, suggests a self-eclipsing geometry. We derive a lower limit on the distance of d >∼ 250 pc.