bronchiole
发表于 2025-3-30 09:18:25
https://doi.org/10.1007/978-3-030-58144-2The present status of the period studies of cataclysmic variables is briefly reviewed, mainly from the observational point of view. A few comments on individual objects include EM Cyg, Z Cha, WZ Sge and AM CVn.
错
发表于 2025-3-30 14:25:24
https://doi.org/10.1007/978-3-030-58969-1We describe a method for imaging the accretion disc of a Cataclysmic Variable star. We use the two-dimensional information contained in the line profiles as they vary with phase to invert the line formation process. Asymmetries in the disc, as are caused by the bright-spot, for example, are accounted for naturally.
起草
发表于 2025-3-30 19:41:34
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indubitable
发表于 2025-3-30 21:12:31
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neuron
发表于 2025-3-31 01:17:59
The Periods of Cataclysmic VariablesThe present status of the period studies of cataclysmic variables is briefly reviewed, mainly from the observational point of view. A few comments on individual objects include EM Cyg, Z Cha, WZ Sge and AM CVn.
可行
发表于 2025-3-31 08:52:34
Mapping the Line Emission Distribution of Cataclismic Variable StarsWe describe a method for imaging the accretion disc of a Cataclysmic Variable star. We use the two-dimensional information contained in the line profiles as they vary with phase to invert the line formation process. Asymmetries in the disc, as are caused by the bright-spot, for example, are accounted for naturally.
chalice
发表于 2025-3-31 09:40:38
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松紧带
发表于 2025-3-31 15:40:18
Multi-Wavelength Observations of Dwarf Novae During Outburstst. Six objects were caught during the rise, and a short flare was detected in SU UMa. It lasted 20 hours and reached a maximum increase of 3.6 in flux at 5500 A. The flare was simultaneous at all observed wavelengths.
他一致
发表于 2025-3-31 18:01:33
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乳白光
发表于 2025-3-31 22:29:58
Tiago H. Moreira de Oliveira,Marco Painholysmic variables have been identified and new observations of one already known object have been accumulated. Observations in the visible and UV-region show variability and differences in spectral type.If compared to the numbers of cataclysmic variables/white dwarfs as computed by Ritter and Burkert (1985)there is a shortage of a factor of 5.