FORAY
发表于 2025-3-21 17:38:25
书目名称Cataclysmic Variables and Related Objects影响因子(影响力)<br> http://impactfactor.cn/2024/if/?ISSN=BK0222414<br><br> <br><br>书目名称Cataclysmic Variables and Related Objects影响因子(影响力)学科排名<br> http://impactfactor.cn/2024/ifr/?ISSN=BK0222414<br><br> <br><br>书目名称Cataclysmic Variables and Related Objects网络公开度<br> http://impactfactor.cn/2024/at/?ISSN=BK0222414<br><br> <br><br>书目名称Cataclysmic Variables and Related Objects网络公开度学科排名<br> http://impactfactor.cn/2024/atr/?ISSN=BK0222414<br><br> <br><br>书目名称Cataclysmic Variables and Related Objects被引频次<br> http://impactfactor.cn/2024/tc/?ISSN=BK0222414<br><br> <br><br>书目名称Cataclysmic Variables and Related Objects被引频次学科排名<br> http://impactfactor.cn/2024/tcr/?ISSN=BK0222414<br><br> <br><br>书目名称Cataclysmic Variables and Related Objects年度引用<br> http://impactfactor.cn/2024/ii/?ISSN=BK0222414<br><br> <br><br>书目名称Cataclysmic Variables and Related Objects年度引用学科排名<br> http://impactfactor.cn/2024/iir/?ISSN=BK0222414<br><br> <br><br>书目名称Cataclysmic Variables and Related Objects读者反馈<br> http://impactfactor.cn/2024/5y/?ISSN=BK0222414<br><br> <br><br>书目名称Cataclysmic Variables and Related Objects读者反馈学科排名<br> http://impactfactor.cn/2024/5yr/?ISSN=BK0222414<br><br> <br><br>
Resistance
发表于 2025-3-21 23:24:58
The Nova-Likes Ac Cnc, Rw Tri, Ux Uma and the Nova Dq Her: Common and Different Propertiesysis is based on simultaneous high-speed UBVRI photometry, covering several dozens of orbital cycles evenly distributed over 14 years (1982...1995) for DQ Her, and over 11 years (1985...1995) for the other three stars. All data have been obtained with the 1.25 m telescope at the Crimean Astrophysica
LARK
发表于 2025-3-22 01:47:53
http://reply.papertrans.cn/23/2225/222414/222414_3.png
脆弱么
发表于 2025-3-22 08:00:14
Applications of Indirect Accretion Disc Imaging to Orbital Solutions for Primary Stars is a problem for which there is no universally applicable solution. Velocity measurements are handicapped because the accretion disc about the primary often dominates the optical spectrum. Therefore spectroscopists resort to measuring line profile symmetry in individual spectra of the accretion dis
cavity
发表于 2025-3-22 10:25:52
http://reply.papertrans.cn/23/2225/222414/222414_5.png
啮齿动物
发表于 2025-3-22 15:45:54
Studies in Flickering bother studying this ‘noise’? Three reasons come to mind: (i) flickering is a fundamental signature of accretion, to the point of being a necessary characteristic (if it doesn’t flicker, it’s not a CV); (ii) energetically, flickering is not a small effect and can contribute up to a few tens of perc
啮齿动物
发表于 2025-3-22 17:55:45
Decomposing Interacting Binary Light Curves: The Eclipses of the Mean Light, Secular Variability andnes 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.
弯腰
发表于 2025-3-22 23:08:23
The Place of Origin of the Flickering in Z Cha(iv) scintillation (negligible) and (v) any residual noise. Calculating the rms-scatter of the count rates in a light curve as a function of orbital phase, ø, through accretion disk eclipse of high inclination CVs — after subtraction of a smoothed light curve to remove orbital and long-term variatio
无节奏
发表于 2025-3-23 02:50:25
TT Ari-94: A Study of 1.6...60 Minute Variabilityy range 10...900 cycle d. are found. The highest peaks in the power spectrum cover the wide range of 28...139 cycle d.. Variations occur at a few preferred time-scales rather than at one cycle length, with a possible secular decrease. In the frequency range 90...900 cycle d. the power spectrum obeys
Gustatory
发表于 2025-3-23 09:06:31
Time Resolved Optical Spectroscopy of V795 Herurce 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 Hß and Hγ line wings (extending to ~1800kms.) is present, with complex asymmetric properties.