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Titlebook: Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments; Proceedings of IAU C H. Drechsel,Y. Kondo,J. Rahe

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樓主: TEMPO
11#
發(fā)表于 2025-3-23 10:21:16 | 只看該作者
12#
發(fā)表于 2025-3-23 15:04:40 | 只看該作者
https://doi.org/10.1007/978-3-030-58872-4pass through the observed light centre of the bright spot eclipse. The light centre is defined as the point corresponding to the half flux points in the ingress and egress of the eclipse of the compact part of the bright spot. The theoretical stream width indicates that the centre of the stream must intersect the bright spot close to this point.
13#
發(fā)表于 2025-3-23 21:29:46 | 只看該作者
14#
發(fā)表于 2025-3-24 02:10:08 | 只看該作者
,The “Return” from the Transcendental,ge during quiescence. A delay in the progress of normal outbursts toward higher frequencies confirms the delay, seen with IUE, in the onset of a normal outburst toward higher frequencies. Just after outburst, the system is substantially bluer than later in quiescence.
15#
發(fā)表于 2025-3-24 04:51:29 | 只看該作者
16#
發(fā)表于 2025-3-24 08:07:22 | 只看該作者
17#
發(fā)表于 2025-3-24 10:59:47 | 只看該作者
Observations of Eclipsing Dwarf Novaepass through the observed light centre of the bright spot eclipse. The light centre is defined as the point corresponding to the half flux points in the ingress and egress of the eclipse of the compact part of the bright spot. The theoretical stream width indicates that the centre of the stream must intersect the bright spot close to this point.
18#
發(fā)表于 2025-3-24 16:15:22 | 只看該作者
19#
發(fā)表于 2025-3-24 20:23:40 | 只看該作者
Long-Term Optical Photometry of the Dwarf Nova VW HYIge during quiescence. A delay in the progress of normal outbursts toward higher frequencies confirms the delay, seen with IUE, in the onset of a normal outburst toward higher frequencies. Just after outburst, the system is substantially bluer than later in quiescence.
20#
發(fā)表于 2025-3-25 00:55:34 | 只看該作者
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