The Most Massive White Dwarfs in the Solar Neighborhood
arXiv:2103.06906 · doi:10.1093/mnras/stab767
Abstract
We present an analysis of the most massive white dwarf candidates in the Montreal White Dwarf Database 100 pc sample. We identify 25 objects that would be more massive than if they had pure H atmospheres and CO cores, including two outliers with unusually high photometric mass estimates near the Chandrasekhar limit. We provide follow-up spectroscopy of these two white dwarfs and show that they are indeed significantly below this limit. We expand our model calculations for CO core white dwarfs up to , which corresponds to the high-density limit of our equation-of-state tables, g cm. We find many objects close to this maximum mass of our CO core models. A significant fraction of ultramassive white dwarfs are predicted to form through binary mergers. Merger populations can reveal themselves through their kinematics, magnetism, or rapid rotation rates. We identify four outliers in transverse velocity, four likely magnetic white dwarfs (one of which is also an outlier in transverse velocity), and one with rapid rotation, indicating that at least 8 of the 25 ultramassive white dwarfs in our sample are likely merger products.
MNRAS, in press
References in corpus (13)
- On the Spectral Evolution of Hot White Dwarf Stars. I. A Detailed Model-Atmosphere Analysis of Hot White Dwarfs from SDSS DR12
- Binary Star Origin of High Field Magnetic White Dwarfs
- On the Spectral Evolution of Cool, Helium-Atmosphere White Dwarfs: Detailed Spectroscopic and Photometric Analysis of DZ Stars
- On the Measurement of Fundamental Parameters of White Dwarfs in the Gaia Era
- The 100 pc White Dwarf Sample in the SDSS Footprint
- white dwarfs within 40 pc II: the volume-limited northern hemisphere sample
- Evolutionary Models for the Remnant of the Merger of Two Carbon-Oxygen Core White Dwarfs
- A New Generation of Cool White Dwarf Atmosphere Models. IV. Revisiting the Spectral Evolution of Cool White Dwarfs
- white dwarfs within 40 pc I: spectroscopic observations of new candidates
- Merging Binary Stars and the magnetic white dwarfs
- An ultra-massive white dwarf with a mixed hydrogen-carbon atmosphere as a likely merger remnant
- Discovery of a hot ultramassive rapidly rotating DBA White Dwarf
- Intermediate-Mass Stars Become Magnetic White Dwarfs
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