On planetary nebula nuclei of the spectral type 'continuous'

Details On planetary nebula nuclei of the spectral type 'continuous' On planetary nebula nuclei of the spectral type 'continuous'

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasp..106...56f&link_type=abstract

Publications of the Astronomical Society of the Pacific, vol. 106, no. 695, p. 56-58

Astronomy and Astrophysics

Astronomy

7

Absorption Spectra, Continuous Radiation, Photosphere, Planetary Nebulae, Spectrum Analysis, Stellar Atmospheres, Stellar Radiation, Stellar Spectra, Astronomical Spectroscopy, Continuums, Helium, Hydrogen, Iron, Iue, Nitrogen, Oxygen

Scientific paper

A detailed reexamination of existing and new International Ultraviolet Explorer (IUE) low-and high-resolution spectra, plus a search of recent literature, shows that for most of the central stars of planetary nebulae the spectral classification previously called 'continuous-type' does not really exist. The stellar continua show primarily photospheric absorption features of N V, O V, C IV, H, He II, Fe VII, Fe VI, and Fe V, and/or P Cygni profiles.

Affiliated with

Also associated with

No associations

Rating

On planetary nebula nuclei of the spectral type 'continuous' 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 On planetary nebula nuclei of the spectral type 'continuous', we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On planetary nebula nuclei of the spectral type 'continuous' will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1684456