The Nebular Environment and Enigmatic Hard X-Ray Emission of the Hot DO White Dwarf KPD 0005+5106

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The Nebular Environment and Enigmatic Hard X - ray Emission of the Hot DO White Dwarf KPD 0005 + 5106

We have detected an ionized nebula around the hot DO white dwarf KPD0005+5106, and used the [O III]/Hα ratios and nebular velocities to separate this nebula from the background H II region of AO Cas. The angular size of the [O III] nebula of KPD0005+5106 is∼ 3. The velocity of this nebula is similar to those of the local interstellar H I gas and the interstellar/circumstellar absorption lines i...

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ژورنال

عنوان ژورنال: The Astronomical Journal

سال: 2004

ISSN: 0004-6256,1538-3881

DOI: 10.1086/424942