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Time resolved spectroscopy of long-period DQ Herculis stars
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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
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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
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The nebula around the binary post-AGB star 89 Herculis
Astronomy and Astrophysics, 2023Iván Gallardo Cava +2 more
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Parent Stars of Extrasolar Planets. IV. 14 Herculis, HD 187123, and HD 210277
Astrophysical Journal, 1999Steven H Saar
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