We investigated the relationship between the kinematics and mass of young (0.95 M_⊙) are consistent with the expected relative contributions of single star evolution and mergers. We find that the kinematics are consistent with the majority of high-mass white dwarfs being formed through single star evolution
Context. The initial-final mass relationship of white dwarfs, which is poorly constrained, is of par...
We present the fractional distribution of spectroscopic subtypes, range and distribution of surface ...
We revisit the properties and astrophysical implications of the field white dwarf mass distribution ...
This is a pre-copyedited, author-produced PDF of an article accepted for publication in "Monthly Not...
Context. Kinematic and chemical tagging of stellar populations have both revealed much information o...
We use the Sloan Digital Sky Survey Data Release 12, which is the largest availablewhite dwarf catal...
We present the mass distribution, gravitational redshifts, radial velocities, and space motions of w...
We present the kinematical properties, distribution of spectroscopic subtypes, and stellar populatio...
]Context] Kinematic and chemical tagging of stellar populations have both revealed much information ...
Original article can be found at: http://www.aanda.org/--Copyright The European Southern Observatory...
We present the kinematics of a sample of 398 DA white dwarfs from the SPY project (ESO SN Ia Progen...
Context.The initial-final mass relationship of white dwarfs, which is poorly constrained, is of para...
Intermediate mass stars either end their lives as a white dwarf (WD) or a neutron star, depending al...
Context. The initial-final mass relationship of white dwarfs, which is poorly constrained, is of par...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/361.html Copyright ASPWe present...
Context. The initial-final mass relationship of white dwarfs, which is poorly constrained, is of par...
We present the fractional distribution of spectroscopic subtypes, range and distribution of surface ...
We revisit the properties and astrophysical implications of the field white dwarf mass distribution ...
This is a pre-copyedited, author-produced PDF of an article accepted for publication in "Monthly Not...
Context. Kinematic and chemical tagging of stellar populations have both revealed much information o...
We use the Sloan Digital Sky Survey Data Release 12, which is the largest availablewhite dwarf catal...
We present the mass distribution, gravitational redshifts, radial velocities, and space motions of w...
We present the kinematical properties, distribution of spectroscopic subtypes, and stellar populatio...
]Context] Kinematic and chemical tagging of stellar populations have both revealed much information ...
Original article can be found at: http://www.aanda.org/--Copyright The European Southern Observatory...
We present the kinematics of a sample of 398 DA white dwarfs from the SPY project (ESO SN Ia Progen...
Context.The initial-final mass relationship of white dwarfs, which is poorly constrained, is of para...
Intermediate mass stars either end their lives as a white dwarf (WD) or a neutron star, depending al...
Context. The initial-final mass relationship of white dwarfs, which is poorly constrained, is of par...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/361.html Copyright ASPWe present...
Context. The initial-final mass relationship of white dwarfs, which is poorly constrained, is of par...
We present the fractional distribution of spectroscopic subtypes, range and distribution of surface ...
We revisit the properties and astrophysical implications of the field white dwarf mass distribution ...
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