The ISO-SWS Line Spectrum of Planetary Nebula NGC 7027

Details The ISO-SWS Line Spectrum of Planetary Nebula NGC 7027 The ISO-SWS Line Spectrum of Planetary Nebula NGC 7027

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456..175b&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Computer Science

Stars: Abundances-, Tars: Planetary Nebulae: Individual: Ngc 7027-, Nfrared:Ism: Lines And Bands

Scientific paper

We present the spectrum of the brightest planetary nebula NGC 7027 as was observed by the Short Wavelength Spectrometer (SWS), on board the Infrared Space Observatory (ISO). These data allows us to derive the electron density, and in conjunction with the IUE and optical spectra, we have derived the electron temperature for several ions. The nebular composition has been determined, and a discussion of the evolutionary status of the central star is given.

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