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The DQ Herculis stars

Publications of the Astronomical Society of the Pacific, 1994
We review the properties of the DQ Herculis stars: cataclysmic variables containing an accreting, magnetic, rapidly rotating white dwarf. These stars are characterized by strong X-ray emission, high-excitation spectra, and very stable optical and X-ray pulsations in their light curves. There is considerable resemblance to their more famous cousins, the
Joseph Patterson
exaly   +2 more sources

The nebula around the binary post-AGB star 89 Herculis

Astronomy and Astrophysics, 2023
Iván Gallardo Cava   +2 more
exaly  

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