Visitors from the Halo: 11 Gyr old White Dwarfs in the Solar Neighborhood
Mukremin Kilic, Jeffrey A. Munn, Kurtis A. Williams, P. M. Kowalski,, Ted von Hippel, Hugh C. Harris, Elizabeth J. Jeffery, Steven DeGennaro,, Warren R. Brown, B. McLeod

TL;DR
This paper reports the discovery of three nearby old halo white dwarfs, including a binary system, using proper motion surveys and follow-up spectroscopy, indicating they are among the oldest known field white dwarfs and useful for constraining Galactic ages.
Contribution
The study identifies and characterizes the oldest halo white dwarfs using a large proper motion survey, demonstrating the potential of deep imaging surveys to find ancient stellar remnants.
Findings
Three old halo white dwarf candidates discovered within 80 pc.
Spectroscopic analysis shows hydrogen atmospheres with temperatures 3700-4100 K.
Estimated ages of 10-11 Gyr for these white dwarfs.
Abstract
We report the discovery of three nearby old halo white dwarf candidates in the Sloan Digital Sky Survey (SDSS), including two stars in a common proper motion binary system. These candidates are selected from our 2800 square degree proper motion survey on the Bok and U.S. Naval Observatory Flagstaff Station 1.3m telescopes, and they display proper motions of 0.4-0.5 arcsec/yr. Follow-up MMT spectroscopy and near-infrared photometry demonstrate that all three objects are hydrogen-dominated atmosphere white dwarfs with Teff = 3700 - 4100 K. For average mass white dwarfs, these temperature estimates correspond to cooling ages of 9-10 Gyr, distances of 70-80 pc, and tangential velocities of 140-200 km/s. Based on the UVW space velocities, we conclude that they most likely belong to the halo. Furthermore, the combined main-sequence and white dwarf cooling ages are 10-11 Gyr. Along with SDSS…
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