Measuring The Mass-Radius Relation of White Dwarfs Using Wide Binaries
Measuring the mass-radius relation of individual white dwarfs is an empirically challenging task that has been performed for only a few dozen stars. We measure the white dwarf mass-radius relation using gravitational redshifts and radii of 137 white dwarfs in wide binaries with main sequence compani...
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| creator | Arseneau, Stefan Chandra, Vedant Hwang, Hsiang-Chih Zakamska, Nadia L Pallathadka, Gautham Adamane Crumpler, Nicole R Hermes, J J El-Badry, Kareem Hans-Walter Rix Stassun, Keivan G Gaensicke, Boris T Brownstein, Joel R Morrison, Sean |
| description | Measuring the mass-radius relation of individual white dwarfs is an empirically challenging task that has been performed for only a few dozen stars. We measure the white dwarf mass-radius relation using gravitational redshifts and radii of 137 white dwarfs in wide binaries with main sequence companions. We obtain the space velocities to these systems using the main sequence companion, and subtract these Doppler redshifts from the white dwarfs' apparent motions, isolating their gravitational redshifts. We use Gaia data to calculate the surface temperatures and radii of these white dwarfs, thereby deriving an empirical gravitational redshift-radius relation. This work demonstrates the utility of low-resolution Galactic surveys to measure the white dwarf equation of state. Our results are consistent with theoretical models, and represent the largest sample of individual white dwarf gravitational redshift measurements to date. |
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| subjects | Equations of state Red shift White dwarf stars |
| title | Measuring The Mass-Radius Relation of White Dwarfs Using Wide Binaries |
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