Discovery of an O VI-emitting Nebula around the Hot White Dwarf KPD 0005+5106

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Published 2004 April 15 © 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Birgit Otte et al 2004 ApJ 606 L143 DOI 10.1086/421397

1538-4357/606/2/L143

Abstract

A survey of diffuse interstellar sight lines observed with the Far Ultraviolet Spectroscopic Explorer has led to the serendipitous discovery of a high-ionization nebula around the hot white dwarf KPD 0005+5106. The nebula has an O VI λ1032 surface brightness of up to 25,000 photons s-1 cm-2 sr-1, making it the brightest region of extended O VI emission in our survey. Photoionization models using the incident white dwarf continuum successfully reproduce the observed O VI intensity. The O VI emission arises in the highly ionized inner region of a planetary nebula around KPD 0005+5106. This newly discovered nebula may be one member of a class of high-ionization planetary nebulae that are difficult to detect in the optical, but that can be easily identified in the ultraviolet.

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10.1086/421397