The dwarf nova RX Volantis in Quiescence

Physics

Scientific paper

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Stars: Spectroscopy, Stars: Variables: Cataclysmic Variables

Scientific paper

We present the first optical spectrum of the dwarf nova RX Vol. The system is found at a magnitude of R=20.0. Its spectrum is dominated by Balmer lines and HeI in emission, as expected for a low mass transfer system situated below the period gap. We tentatively derive a disc temperature around 8000K with moderate density. It is seen at low inclination.

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