[PDF] Top 20 The mass of the white dwarf in GW Libra
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The mass of the white dwarf in GW Libra
... The population of cataclysmic variables (CVs) provides an important sample of binary systems possessing homogeneous configurations of white dwarfs (WDs) accreting from near main-sequence donor stars. A CV ... See full document
17
Mass and eccentricity constraints on the planetary debris orbiting the white dwarf WD 1145+017
... Our N-body numerical simulations are based on a model of WD 1145 + 017 that, while taking into account the results from the recent follow-up observations, ignores the detailed process of the tidal disruption of the ... See full document
9
Precise mass and radius values for the white dwarf and low mass M dwarf in the pre cataclysmic binary NN Serpentis
... theoretical mass-radius relation for very low mass ...initial-final mass relation could be used to estimate the age of NN Ser, but since the system has passed through a common envelope phase its ... See full document
21
The mass of the white dwarf in the old nova BT Mon
... massive white dwarfs, while slower TNRs occur on lower mass white ...the mass of the white dwarf, we are motivated to try to measure the masses of novae as a ... See full document
18
The white dwarf initial–final mass relation for progenitor stars from 0 85 to 7 5 M ⊙
... Wide white dwarf main sequence binaries have also been used ( Catalán et ...low mass, and ages derived from a single main sequence companion have errors far larger than those of star ...of ... See full document
15
An accurate mass and radius measurement for an ultracool white dwarf
... The mass-radius plot for low-mass stars is shown in Fig- ure ...measured mass and radius of the low-mass star in SDSS 0138-0016 are consistent with evolutionary mod- ...precise ... See full document
10
The post outburst pulsations of the accreting white dwarf in the cataclysmic variable GW Librae
... air mass (assuming a plane parallel atmosphere), and the flux ratio was simultaneously fitted over the six nights for air masses 1 – ...of GW Librae remains constant to a level much better than the ∼10% ... See full document
11
Relativistic deflection of background starlight measures the mass of a nearby white dwarf star
... the white dwarf Stein 2051 ...the mass of Stein 2051 B —the sixth nearest white dwarf to the Sun—as ...This mass determination provides confirmation of the physics of degenerate ... See full document
34
Asymmetric mass-loss from the white dwarf WD 0253+209 : Secret revealed
... this white dwarf is extremely low. The spectral index of this white dwarf in V band is ...this white dwarf is relatively colder. In the catalog, this white dwarf is ... See full document
7
The field white dwarf mass distribution
... to white dwarfs found in the cooling age range ...being white dwarfs based on colours and ...DA white dwarfs, and we define the com- pleteness as the fraction of objects with a spectrum among those ... See full document
16
Unstable low mass planetary systems as drivers of white dwarf pollution
... after mass loss results in delivery of material to the WD over a period of a few hundred ...following mass loss, and then an instability among the planets just before ...stellar mass loss and the ... See full document
18
The Dynamics of White Dwarfs, Black Holes and Stellar Cusps
... Cusp Profile: One of the major factors in determining the rates is the stellar distribution. In our simulations we use an η-model (Tremaine et al., 1994) of a spherical stellar cusp with a central SMBH to establish the ... See full document
193
The white dwarf binary pathways survey – I a sample of FGK stars with white dwarf companions
... two white dwarfs of arbitrarily mass, which would cause a spread in the luminosities of SN Ia, affecting their use as stan- dard ...a white dwarf stably accretes material from a non-degenerate ... See full document
13
An overview of white dwarf stars
... massive white dwarfs have larger internal densities (for comparable temperatures) and, therefore, develop a crystallized core earlier, at higher luminosities or, equivalently, higher effective ...black ... See full document
10
Eclipsing white dwarf binaries
... theoretical mass-radius relations, which are used in a wide range of astrophysical circumstances such as inferring accurate masses and radii of transiting exoplanets, calibrating stellar evolutionary models and ... See full document
205
Information and Cosmological Objects
... the white dwarfs consisting of carbon and oxygen with helium-hydrogen shell [7, ...of white dwarfs ...prescribed mass) and the loss of heat resulting from non-degenerate component of the substance ... See full document
13
A double white dwarf with a paradoxical origin?
... low-mass white dwarfs present us with an intriguing puzzle. The secondary white dwarf has a mass just over 1 M , which is near the threshold separating white dwarfs with a ... See full document
9
WHITE DWARF PERIOD TABLES
... (pre-)white dwarf pulsators into DOV and PNNV classes have become obsolete, and now the denomination GW Vir stars is used instead for all the post-AGB stars showing nonradial g-mode pulsations ... See full document
31
Pulsating white dwarfs
... the mass of the white dwarf. Most white dwarfs have atmospheres dominated by H, and the remainder by ...the white dwarf cools. The He-core white dwarf stars in the ... See full document
9
Detection of a white dwarf companion to the white dwarf SDSSJ125733 63+542850 5
... two white dwarf model spectra drawn from the same model grids as in ...massive white dwarf, 500 < v sin i < 1750 km s −1 , in steps ... See full document
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