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• W2149114598 abstract "BD +30 3639, the brightest planetary nebula at X-ray energies, was observed with Suzaku, an X-ray observatory launched on 2005 July 10. Using the X-ray Imaging Spectrometer, the K lines from C VI, O VII, and O VIII were resolved for the first time, and the C/O, N/O, and Ne/O abundance ratios were determined. The C/O and Ne/O abundance ratios exceed the solar value by factors of at least 30 and 5, respectively. These results indicate that the X-rays are emitted mainly by helium-shell-burning products." @default.
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• W2149114598 date "2006-08-01" @default.
• W2149114598 modified "2023-09-30" @default.
• W2149114598 title "Suzaku Reveals Helium-burning Products in the X-Ray-emitting Planetary Nebula BD +30 3639" @default.
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• W2149114598 doi "https://doi.org/10.1086/507465" @default.
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