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

  • Published:2004-11 Issue:5 Volume:128 Page:2357-2363
  • ISSN:0004-6256
  • Container-title:The Astronomical Journal
  • language:en
  • Short-container-title:Astron J

Author:

Chu You-Hua,Gruendl Robert A.,Williams Rosa M.,Gull Theodore R.,Werner Klaus

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 15 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Hard X-Ray Emission Associated with White Dwarfs. IV. Signs of Accretion from Substellar Companions;The Astrophysical Journal;2021-04-01

2. Far-UV spectroscopy of two extremely hot, helium-rich white dwarfs;Astronomy & Astrophysics;2017-04-19

3. Challenges faced by current Galactic planetary nebula surveys;Proceedings of the International Astronomical Union;2016-10

4. The H  surface brightness-radius relation: a robust statistical distance indicator for planetary nebulae;Monthly Notices of the Royal Astronomical Society;2015-11-18

5. On the distances of planetary nebulae;Monthly Notices of the Royal Astronomical Society;2015-04-08
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