Constraints on the system parameters of the dwarf nova AH Herculis

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Dwarf Novae, Orbital Elements, Spectrum Analysis, Stellar Spectrophotometry, Ubv Spectra, Electrophotometry, Light Curve, Main Sequence Stars, Periodic Variations, Stellar Color, Stellar Magnitude, Stellar Mass

Scientific paper

It is noted that no periodic variations with time scales of minutes or hours could be detected in the present photoelectric UBV observations of AH Her. An orbital period of 5.9 + or - 0.5 h is derived from the decline rate after outbursts, as well as the colors in quiescence. The estimates of orbital inclination, mass and system dimensions presented can only be improved by detailed spectroscopic study with high time resolution, in order to obtain a radial velocity curve of the system's primary and secondary.

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