The Complex IUE Spectrum of the ``O VI Sequence'' Planetary Nebula NGC 2867

Details The Complex IUE Spectrum of the ``O VI Sequence'' Planetary Nebula NGC 2867 The Complex IUE Spectrum of the ``O VI Sequence'' Planetary Nebula NGC 2867

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apjs..114..263f&link_type=abstract

Astrophysical Journal Supplement, v.114, p.263

Astronomy and Astrophysics

Astronomy

6

Ultraviolet: Ism, Ism: Planetary Nebulae: Individual Ngc Number: Ngc 2867, Stars: Mass Loss

Scientific paper

The IUE spectrum of the planetary nebula NGC 2867 and its central star displays a rich variety of emission lines that has not been reported before. Fluxes for more than 80 UV features were determined from low- and high-dispersion spectra. Electron densities of log Ne = 3.4 +/- 0.1 cm-3 from C III], log Ne = 3.9 +/- 0.2 cm-3 from [Ne IV], and log Ne = 3.25 +/- 0.2 cm-3 from O IV] diagnostics were derived. Detection of O VIII lines (I.P. = 871 eV) are thought to require a corona or strong stellar winds, yet no strong P Cygni profiles were observed. Several resonantly excited Fe II lines were identified.

Affiliated with

Also associated with

No associations

Rating

The Complex IUE Spectrum of the ``O VI Sequence'' Planetary Nebula NGC 2867 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 The Complex IUE Spectrum of the ``O VI Sequence'' Planetary Nebula NGC 2867, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Complex IUE Spectrum of the ``O VI Sequence'' Planetary Nebula NGC 2867 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1223662