[PDF] Top 20 The Murky Origin of Snow White and Her T-Even Dwarfs
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The Murky Origin of Snow White and Her T-Even Dwarfs
... the T-even phages originated The materials used in our experiments consisted of the has historical significance and is of scientific conse- same bacterial ... See full document
6
Observations of remnant planetary systems at white dwarfs
... the white dwarf of ≈ (6 ...DA white dwarfs (Vennes et ...and origin of the debris around SDSS J1617+1620 remain limited as only two photospheric elements are so far ... See full document
146
The properties of cool DZ white dwarfs
... The SDSS spectra obtained using the original spectrograph (released DR1– DR8) show very good flux calibration as synthetic g, r, and i magnitudes calculated from these spectra agree well with SDSS photometry. This has ... See full document
253
The Genesis of Magnetic Fields in White Dwarfs
... magnetic white dwarfs with detached, non-degenerate companions?” This question is awaiting an answer and thus the pro- genitors of the MCVs still need to be ...binary origin of magnetic fields in ... See full document
167
A new magnetic white dwarf: PG 2329+267
... the origin of the magnetic field in PG 2329+267, we can find evidence both for and against the hypothesis that it evolved from a chemically peculiar, magnetic Ap or Bp ...of white dwarfs, suggesting ... See full document
5
On the evolution of magnetic white dwarfs
... the origin of HFMWDs, accounting for their mass, velocity, and magnetic fi eld strength ...the white dwarf ...two white dwarfs or a white dwarf and the core of a giant star ( García- ... See full document
13
Infrared variability of two dusty white dwarfs
... single white dwarf discovered to display excess infrared emission ( Zuckerman & Becklin 1987 ) , and follow-up studies have shown that the excess fl ux arises from a close-in hot dust disk ( Graham et ...The ... See full document
13
Interpretation and diversity of exoplanetary material orbiting white dwarfs
... for white dwarf atmospheres is also re- quired, and the diffusion processes operating therein are an active area of research (Bauer & Bildsten 2018; Cunningham et ...of white dwarfs is presently ... See full document
17
The Dynamics of White Dwarfs, Black Holes and Stellar Cusps
... velocity white dwarfs in SDSS is a statistical anomaly, since the number of objects is ...the white dwarf GD 50, has a velocity and cooling age consistent with a Pleiades origin (Dobbie et ... See full document
193
The gaseous component to planetary debris discs at white dwarfs
... the white dwarf, this indicates that we only see the emission when it is on the far side of its orbit around the white dwarf with respect to our line of ...the white dwarf, whereas the maximum ... See full document
189
Cold giant planets evaporated by hot white dwarfs
... WD 0512 + 326 ( 14 Aur C ) is a F2V + DA ( Vennes et al. 1998 ) binary which is part of the complex multiple system 14 Aur. There is some confusion in the literature regarding the make-up of this system. The most ... See full document
9
Tidal circularization of gaseous planets orbiting white dwarfs
... K2 white dwarf planet occurence rates through tran- sit photometry as a function of mass and ...orbiting white dwarfs through as- trometry (Perryman et ... See full document
15
Pure helium 3D model atmospheres of white dwarfs
... the grid resolution, artificial viscosity, geometrical dimen- sions, and numerical schemes for the hydrodynamics solver (see Table 3 of Tremblay et al. (2013a) for more detail). This work relies on the same numerical ... See full document
18
The Gaia DR1 mass–radius relation for white dwarfs
... all white dwarfs that are directly in Gaia DR1, does not allow us to build a meaningful sample of wide ...of white dwarfs that are in common proper motion pairs with Hipparcos or Tycho-2 stars ... See full document
14
Orbital relaxation and excitation of planets tidally interacting with white dwarfs
... a white dwarf and planet include the prospect of the for- mation of second- or third-generation planets, which may even arise from second- or third-generation debris discs (Perets 2011; Schleicher & ... See full document
21
Outbursts in two new cool pulsating DA white dwarfs
... One complication in our extraction came from the presence of charge bleed in the K2 target pixels caused by the saturation of naked-eye M dwarf, 82 Virginis ( also known as the variable m Vir, J134136.78 − 084210.7 ) , ... See full document
12
The onset of convective coupling and freezing in the white dwarfs of 47 Tucanae
... to even fainter magnitudes, the agreement between models and the data remains good and the data agree somewhat better with the frozen evolution (solid black curve), yielding a hint that indeed the white ... See full document
7
Survivability of radio loud planetary cores orbiting white dwarfs
... As the field of post-main-sequence planetary system sci- ence grows, so does the need for models which can assess the likelihood of discovering planets at particular locations and with particular physical properties. In ... See full document
13
The Last Fairy Tale
... found Snow White in the bathroom one night. I heard her get up to leave, but I spent the rest of the night running away from the man with the grey ...but her little store has been ratted out ... See full document
12
White Dwarfs are Small, Fast-Spinning Hot Stars
... There are more than 270 links in 14 tables, leading towards the database, in which a reader can check the source of information (reference). The goal of this is not to dispute or to support the mainstream points of view, ... See full document
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