Metals in Cool DA White Dwarfs*

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Published 1998 August 31 © 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation B. Zuckerman and I. Neill Reid 1998 ApJ 505 L143 DOI 10.1086/311608

1538-4357/505/2/L143

Abstract

We used the HIRES echelle spectrograph on the Keck telescope to search for metals in the 3700-5200 Å spectra of white dwarfs with hydrogen-rich photospheres. The most popular models that account for the presence of metals are interstellar accretion and comet impact. The data are not easily reconciled with either model, but binarity might play a role. We comment on the implications for Oort-like comet clouds and certain types of planets around main-sequence stars.

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Footnotes

  • Based on observations at the W. M. Keck Observatory.

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10.1086/311608