Results 21 to 30 of about 49 (48)
Stochastic Optical Variability and an rms–Flux Relation in the Intermediate Polar EP240309a
The Astrophysical Journal Supplement SeriesMagnetic cataclysmic variables provide a natural laboratory for studying how accretion interacts with compact-object magnetospheres and generates stochastic variability.
S.-Y. Wu +20 more
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The Astrophysical JournalWe present the first discovery of small-amplitude (tens of millimagnitudes), short-duration (several hours) episodic brightenings in the Transiting Exoplanet Survey Satellite (TESS) light curve of the intermediate polar PBC J0801.2–4625 that are strongly
Vishal Joshi, Akash Sundriyal
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H2215-086 -King of the DQ Herculis stars
The Astrophysical Journal, 1983 J. Patterson, J. E. Steiner
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Formation of high-field magnetic white dwarfs from common envelopes. [PDF]
Proc Natl Acad Sci U S A, 2011 Nordhaus J +4 more
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MAGELLANIC CLOUDS. XII. OBSERVATIONS OF A NOVA IN THE SMALL CLOUD. [PDF]
Proc Natl Acad Sci U S A, 1954 Smith HJ.
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MAGELLANIC CLOUDS. XI. SURVEY OF THE NOVAE. [PDF]
Proc Natl Acad Sci U S A, 1954 Henize KG, Hoffleit D, Nail VM.
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Notes on Binary Stars: IV. A Source of Spurious Eccentricity in Spectroscopic Binaries. [PDF]
Proc Natl Acad Sci U S A, 1941 Sterne TE.
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Time resolved spectroscopy of long-period DQ Herculis stars
The Astrophysical Journal, 1985 openaire +1 more source
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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, 2023I Gallardo Cava +2 more
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