Variability of Soft X-Ray Emission of Ex Hydrae Observed with Einstein Observatory
- 1 January 1982
- book chapter
- Published by Springer Nature
Abstract
No abstract availableKeywords
This publication has 23 references indexed in Scilit:
- A model for the X-ray emitting cataclysmic variable EX HydraeThe Astrophysical Journal, 1981
- The system AM Her = 4U 1814 + 50Space Science Reviews, 1980
- Spectrophotometry of dwarf novae in the wavelength range 1250-7500 AMonthly Notices of the Royal Astronomical Society, 1980
- The 2 : 3 period ratio in the light curve of EX HydraeMonthly Notices of the Royal Astronomical Society, 1980
- Accretion on to highly magnetized white dwarfsMonthly Notices of the Royal Astronomical Society, 1979
- Rapid oscillations in cataclysmic variables. II - The 63 second oscillation of V533 HerculisThe Astrophysical Journal, 1979
- The HEAO-A2 soft X-ray survey of cataclysmic variable stars: EX Hydrae during optical quiescenceMonthly Notices of the Royal Astronomical Society, 1979
- The Einstein /HEAO 2/ X-ray ObservatoryThe Astrophysical Journal, 1979
- Cyclotron emission from accreting magnetic white dwarfsMonthly Notices of the Royal Astronomical Society, 1977
- Fourier analysis with unequally-spaced dataAstrophysics and Space Science, 1975