Discovery of New Ultracool White Dwarfs in the Sloan Digital Sky Survey

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Published 2004 August 12 © 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Evalyn Gates et al 2004 ApJ 612 L129 DOI 10.1086/424568

1538-4357/612/2/L129

Abstract

We report the discovery of five new white dwarfs in the Sloan Digital Sky Survey. Four are ultracool, exhibiting strong collision-induced absorption (CIA) from molecular hydrogen and are similar in color to the three previously known coolest white dwarfs, SDSS J1337+00, LHS 3250, and LHS 1402. The fifth star shows milder CIA flux suppression and has a color and spectral shape similar to WD 0346+246. All five new white dwarfs are faint (g > 18.9) and have significant proper motions. One of the new ultracool white dwarfs, SDSS J0947, appears to be in a binary system with a slightly warmer (Teff ~ 5000 K) white dwarf companion.

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10.1086/424568