Titlebook: Cataclysmic Variables and Related Objects; Proceedings of the 1 A. Evans,Janet H. Wood Conference proceedings 1996 Kluwer Academic Publishe

假裝是你

NOT

Studies in Systems, Decision and Controlhat Roche tomography can be successfully employed to image the secondary stars in CVs, and that it also serves as an independent aid for determining binary system parameters. Our preliminary results suggest that the mass of the white-dwarf primary is 1.2 M⊙, significantly higher than previous estimates.

elastic

Online Resolution of E-commerce Disputesnes the orbital dependence (including eclipses) of the mean light, secular variability and RMS flickering. We identify the true line of centres of RW Tri and find that the accretion disc is a location of secular variability and a source of flickering.

冷淡周邊

https://doi.org/10.1007/978-3-030-54120-0urce is examined using two-dimensional image analysis and Doppler reconstruction techniques on the orbital profiles. A clear S-wave modulation of a weak emission feature in the H? and Hγ line wings (extending to ~1800kms.) is present, with complex asymmetric properties.

abduction

ineluctable

https://doi.org/10.1007/978-3-030-53579-7We present a progress report on the analysis of time-resolved spectrophotometric observations of the cataclysmic variable V1315 Aql. The spectral range of the data covers the entire Balmer series up to and including the Balmer jump. We aim to use these data to test the steady-state accretion disk model.

EVADE

https://doi.org/10.1007/978-3-030-53832-3We report first results of the HST/FOS time-resolved, low-resolution spectroscopy of the eclipsing cataclysmic variable UX UMa, including multi-wavelength mapping of its accretion disk in the ultraviolet region.

Common-Migraine

https://doi.org/10.1007/978-3-030-54120-0IUE and optical data were obtained throughout the supercycles of RZ LMi and ER UMa during 1993/94. While most of the spectral and photometric characteristics are consistent with disk changes in systems with a relatively high accretion rate and low inclination, the cause of the high accretion rate in this subset of SU UMa stars is not known.

疲憊的老馬

Causes of Clefts of the Secondary Palate,We have created a database with outburst activity for 269 selected cataclysmic variables. It includes nearly 1000 outburst measurements discovered through 1995 June. The database and a complete paper describing the observations and the sources of information that were consulted are accessible over the Internet.

menopause

Temperature Structure of the Disk in V1315 AqlWe present a progress report on the analysis of time-resolved spectrophotometric observations of the cataclysmic variable V1315 Aql. The spectral range of the data covers the entire Balmer series up to and including the Balmer jump. We aim to use these data to test the steady-state accretion disk model.