J/A+A/307/215 J/A+A/307/215 Spectrophotomety of planetary nebulae F Cuisinier A Acker J Koeppen Astron. Astrophys. 307 215 1996 1996A&A...307..215C V/84 : Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker+, 1992) Planetary nebulae Galaxy: abundances ISM: abundances planetary nebulae: general Spectrohotometric observations at high signal-to-noise ratio for a sample of 62 planetary nebulae are presented, together with the plasma and abundance analyses. The objects were selected homogeneously from the `Strasbourg-ESO Catalogue of Galactic Planetary Nebulae' by their height above the disk (over 300pc) and their H{beta} surface brightness (between 10^-12^ and 10^-14^mW/m^2^/arcsec^2^). The abundances of O, S, Ar, and Cl are tighly correlated. The N/O ratio shows a wide range of values, independent of He or O abundance.

Name PNG name (see in catalogue <V/84>) --- Ident Other name --- Qual Accuracy of the line intensity number=1 For each nebula, the quality class (A, B, C) indicates the accuracy of the line intensities (see Table 1 in the paper) --- 4102 Intensity at 4102A; H I --- 4340 Intensity at 4340A; H I --- 4363 Intensity at 4363A; [O III] --- 4388 Intensity at 4388A; He I --- 4472 Intensity at 4472A; He I --- n_4472 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 4542 Intensity at 4542A; He II --- n_4542 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 4686 Intensity at 4686A; He II --- n_4686 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 4740 Intensity at 4740A; [Ar IV] --- 4861 Intensity at 4861A; H I --- 4922 Intensity at 4922A; He I --- n_4959 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 4959 Intensity at 4959A; [O III] --- n_5007 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 5007 Intensity at 5007A; [O III] --- 5199 Intensity at 5199A; [N I] --- 5412 Intensity at 5412A; He II --- n_5412 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 5518 Intensity at 5518A; [Cl III] --- n_5518 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 5538 Intensity at 5518A; [Cl III] --- n_5538 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 5754 Intensity at 5754A; [N II] --- 5876 Intensity at 5876A; He I --- 6300 Intensity at 6300A; [O I] --- 6312 Intensity at 6312A; [S III] --- 6364 Intensity at 6364A; [O I] --- 6435 Intensity at 6435A; [Ar V] --- 6548 Intensity at 6548A; [N II] --- n_6548 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 6563 Intensity at 6563A; H I --- n_6563 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 6584 Intensity at 6584A; [N II] --- n_6584 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 6678 Intensity at 6678A; He I --- 6716 Intensity at 6716A; [S II] --- n_6716 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 6731 Intensity at 6731A; [S II] --- n_6731 See Note number=2 S: Saturated lines E: Intensities were taken from the Strasbourg-ESO survey spectra (catalogue <V/84>) I: Intensities were estimated from short exposure spectra taken immediately afterwards p: indicates lines that are present in the spectra, but too weak to be measured --- 7006 Intensity at 7006A; [Ar V] --- 7065 Intensity at 7065A; He I --- 7136 Intensity at 7136A; [Ar III] --- 7325 Intensity at 7325A; [O II] --- Simona Mei CDS 1995Sep07 J_A+A_307_215.xml