Ultraviolet spectra of planetary nebulae. VIII - The C/O abundance ratio in the Ring nebula

Details Ultraviolet spectra of planetary nebulae. VIII - The C/O abundance ratio in the Ring nebula Ultraviolet spectra of planetary nebulae. VIII - The C/O abundance ratio in the Ring nebula

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.199p..15f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 199, Apr. 1982, p. 15P-18P.

Astronomy and Astrophysics

Astronomy

6

Abundance, Carbon, Oxygen Ions, Planetary Nebulae, Ultraviolet Astronomy, Ultraviolet Spectra, Electron Energy, Iue, Line Spectra, Spectral Line Width

Scientific paper

The Ring nebula (NGC 6720) has been observed with the International
Ultraviolet Explorer satellite. Measurements of line intensities at a
position on the ring, offset from the central star, lead to a value of
the abundance ratio C/O approximately 1.2, a result which is insensitive
to the adopted value of the electron temperature in the nebula.

Affiliated with

Also associated with

No associations

Rating

Ultraviolet spectra of planetary nebulae. VIII - The C/O abundance ratio in the Ring nebula does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Ultraviolet spectra of planetary nebulae. VIII - The C/O abundance ratio in the Ring nebula, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet spectra of planetary nebulae. VIII - The C/O abundance ratio in the Ring nebula will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-842996