Ultraviolet spectra of planetary nebulae. II - The young planetary nebula IC 4997

Details Ultraviolet spectra of planetary nebulae. II - The young planetary nebula IC 4997 Ultraviolet spectra of planetary nebulae. II - The young planetary nebula IC 4997

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193..511f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 193, Nov. 1980, p. 511-520.

Astronomy and Astrophysics

Astronomy

23

Planetary Nebulae, Ultraviolet Astronomy, Ultraviolet Spectra, Abundance, Electron Density (Concentration), Electron Energy, Iue, Visual Observation

Scientific paper

Observations of the planetary nebula IC 4997 made with the International Ultraviolet Explorer satellite are analyzed in conjunction with visual photoelectric observations. The extinction to the nebula and the electron temperature and density are deduced from the relative intensities of lines emitted by O(+) and O(2+) ions. The relative abundance of C and O is found to be similar to the solar value, whereas the abundances of these elements relative to H are substantially less than solar. The effects of the variability of the nebular emission are considered and found to be only marginally significant.

Affiliated with

Also associated with

No associations

Rating

Ultraviolet spectra of planetary nebulae. II - The young planetary nebula IC 4997 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. II - The young planetary nebula IC 4997, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet spectra of planetary nebulae. II - The young planetary nebula IC 4997 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1391851