X-Rays Reveals Helium-burning Products in Planetary Nebulae with Fast Stellar Winds

Details X-Rays Reveals Helium-burning Products in Planetary Nebulae with Fast Stellar Winds X-Rays Reveals Helium-burning Products in Planetary Nebulae with Fast Stellar Winds

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007asthe.100..444m&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 100, No. 9, p. 444 - 451 (2007)

Astronomy and Astrophysics

Astronomy

X-Rays, Stellar Winds, Planetary Nebulae

Scientific paper

Suzaku observed the X-ray brightest planetary nebula BD+30°3639, and
obtained the C/O, N/O, and Ne/O abundance ratios. The C/O and the Ne/O
abundance ratios exceed the solar value by factors of 85 and 5.8,
respectively. These results indicate that the X-rays are emitted mainly
by helium-shell-burning products.

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