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Magnetic interaction in ultra-compact binary systems

Research in Astronomy and Astrophysics 2009年第7期9卷 725-744页

作者： kinwah wu Mullard Space Science Laboratory University College London Holmbury St. Mary Surrey RH5 6NT United Kingdom

This article reviews the current works on ultra-compact double-degenerate binaries in the presence of magnetic interaction, in particular, unipolar induction. The orbital dynamics and evolution of compact white-dwarf pairs are discussed in detail. Models and predictions of electron cyclotron masers from unipolar-inductor compact binaries and unipolar-inductor white-dwarf planetary systems are presented. Einstein-Laub effects in compact binaries are briefly discussed.

关键词： stars binaries close - stars white dwarfs - gravitational waves - masers - radio continuum stars - X-rays binaries -- planetary systems

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Relativistic reflection X-ray spectra of accretion disks

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Chinese Journal of Astronomy and Astrophysics 2009年第4期9卷 377-389页

作者： Khee-Gan Lee kinwah wu Steven V. Fuerst Graziella Branduardi-Raymont Oliver Crowley Department of Astrophysical Sciences Princeton UniversityPrinceton NJ 08544 USA Mullard Space Science Laboratory University College LondonHolmbury St. Mary Surrey RH5 6NT United Kingdom Kavli Institute for Particle Astrophysics and Cosmology Stanford UniversityStanford CA 94309 USA Department of Physics & Astronomy University College LondonGower Street London WC1E 6BT United Kingdom

We have calculated the relativistic reflection component of the X-ray spectra of accretion disks in active galactic nuclei （AGN）. Our calculations have shown that the spectra can be significantly modified by the motion of the accretion flow, and the gravity and rotation of the central black hole. The absorption edges in the spectra suffer severe en- ergy shifts and smearing, and the degree of distortion depends on the system parameters, in particular, the inner radius of the accretion disk and the disk viewing inclination angles. The effects are significant. Fluorescent X-ray emission lines from the inner accretion disk could be a powerful diagnostic of space-time distortion and dynamical relativistic effects near the event horizons of accreting black holes. However, improper treatment of the reflection component in fitting the X-ray continuum could give rise to spurious line-like features. These features mimic the true fluorescent emission lines and may mask their relativistic signatures. Fully relativistic models for reflection continua together with the emission lines are needed in order to extract black-hole parameters from the AGN X-ray spectra.

关键词： accretion, accretion disks-galaxies active-X-rays galaxies-blackhole physics-relativity

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Photometric observations of three high mass X-ray binaries and a search for variations induced by orbital motion

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Research in Astronomy and Astrophysics 2011年第8期11卷 947-964页

作者： Gordon E. Sarty Bogumil Pilecki Daniel E. Reichart Kevin M. Ivarsen Joshua B. Haislip Melissa C. Nysewander Aaron P. LaCluyze Helen M. Johnston Robert R. Shobbrook Lászl L. Kiss kinwah wu Departments of Psychology and Physics University of Saskatchewan9 Campus DriveSaskatoonSaskatchewan S7N 5A5Canada Warsaw University Observatory Al. Ujazdowskie 400-478 WarsawPoland Universidad de Concepcion Departamento de AstronomaCasilla 160-CConcepcionChile Department of Physics and Astronomy University of North Carolina-Chapel HillCB 3255Phillips HallChapel HillNC 27599-3255USA School of Physics A28 University of SydneyNew South Wales 2006Australia Konkoly Observatory H-1525 BudapestP.O. Box 67Hungary Mullard Space Science Laboratory University College LondonHolmbury St. MaryDorkingSurrey RH5 6NTUnited Kingdom

We searched for long period variation in V-band, It-band and RXTE X-ray light curves of the High Mass X-ray Binaries （HMXBs） LS 1698 / RX J1037.5-5647, HD 110432 / 1H 1249-637 and HD 161103 / RX J1744.7-2713 in an attempt to discover orbitally induced variation. Data were obtained primarily from the ASAS database and were supplemented by shorter term observations made with the 24- and 40-inch ANU telescopes and one of the robotic PROMPT telescopes. Fourier periodograms suggested the existence of long period variation in the V-band light curves of all three HMXBs, however folding the data at those periods did not reveal convincing periodic variation. At this point we cannot rule out the existence of long term V-band variation for these three sources and hints of longer term variation may be seen in the higher precision PROMPT data. Long term V-band observations, on the order of several years, taken at a frequency of at least once per week and with a precision of 0.01 mag, therefore still have a chance of revealing long term variation in these three HMXBs.

关键词： accretion -- stars： Be stars -- stars： neutron stars -- stars： individual LS 1698 HD 110432 HD 161103 -- X-rays： binaries

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