(Ne V) 3426 A line fluxes of planetary nebulae

Details (Ne V) 3426 A line fluxes of planetary nebulae (Ne V) 3426 A line fluxes of planetary nebulae

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105.1287r&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 693, p. 1287-1289

Astronomy and Astrophysics

Astronomy

17

Line Spectra, Neon, Planetary Nebulae, Ultraviolet Astronomy, Ultraviolet Spectra, Helium Ions, Space Observations (From Earth), Spectrophotometers

Scientific paper

We present total (Ne V) 3426 A line fluxes for 23 planetary nebulae and upper limits on this line flux for 21 more objects obtained with a spectrometer system having a 48 arcsec aperture. This emission line is one of the few emission lines arising from the He(+2) regions of nebulae which are accessible by ground-based observations. These whole-nebula line fluxes are needed for the construction of accurate nebular models of highly ionized nebulae.

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