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Supporting Online Material for A Gaseous Metal Disk Around a White Dwarf

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The article was published on 2006-01-01 and is currently open access. It has received 204 citations till now. The article focuses on the topics: White dwarf.

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The Exoplanet Handbook

TL;DR: In this paper, the authors present an overview of the solar system and its evolution, including the formation and evolution of stars, asteroids, and free-floating planets, as well as their internal and external structures.
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Ancient planetary systems are orbiting a large fraction of white dwarf stars

TL;DR: In this article, atmospheric pollution by various elements heavier than helium has been used to infer that a comparable fraction of the white dwarf descendants of such main-sequence stars are orbited by planetary systems, and for plausible planetary system configurations, this total mass is likely to be at least equal to that of the Sun's asteroid belt.
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The chemical diversity of exo-terrestrial planetary debris around white dwarfs

TL;DR: In this article, the authors presented the HST ultraviolet spectra of the white dwarfs PG 0843+516, PG 1015+161, SDSS 1228+1040, and GALEX 1931+0117, which accrete circumstellar planetary debris formed from the destruction of asteroids.
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Magnetic White Dwarfs

TL;DR: In this article, the current status of research on the observational and theoretical characteristics of isolated and binary magnetic white dwarfs (MWDs) is reviewed, and a review of the existing literature is presented.
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疟原虫var基因转换速率变化导致抗原变异[英]/Paul H, Robert P, Christodoulou Z, et al//Proc Natl Acad Sci U S A

宁北芳, +1 more
TL;DR: PfPMP1)与感染红细胞、树突状组胞以及胎盘的单个或多个受体作用,在黏附及免疫逃避中起关键的作�ly.
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Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity

TL;DR: In this article, the authors present analytic formulae that approximate the evolution of stars for a wide range of mass M and metallicity Z, including all phases from the zero-age main sequence up to, and including, the remnant stages.
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Non-LTE line-blanketed model atmospheres of hot stars. 1: Hybrid complete linearization/accelerated lambda iteration method

TL;DR: In this article, a hybrid complete linearization/accelerated lambda iretation (CL/ALI) method was proposed for non-local thermodynamic equilibrium (non-LTE) model stellar atmospheres.
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Are There Unstable Planetary Systems around White Dwarfs

TL;DR: In this article, the authors show that when mass loss is slow, systems of two planets that are marginally stable can become unstable to close encounters, while for three planets the timescale for close approaches decreases significantly with increasing mass ratio.
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