Analysis of chemical abundances in planetary nebulae with [WC] central stars - I. Line intensities and physical conditions

Free Access

Issue		A&A Volume 538, February 2012


Article Number		A54
Number of page(s)		84
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201118217
Published online		01 February 2012

Online material

Table 3

Observed and reddening corrected line ratios (F(Hβ) = 100) and line identifications.

Table 3

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	Fig. 3 Complete MIKE-echelle spectra of Cn 1-5. The most characteristic nebular emission lines have been labelled. Wide stellar WR features, generally stellar helium lines, are clearly visible in some spectral regions.
Open with DEXTER

	Fig. 3 Complete MIKE-echelle spectra of H b4.
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	Fig. 3 Complete MIKE-echelle spectra of He 2-86.
Open with DEXTER

	Fig. 3 Complete MIKE-echelle spectra of M 1-25.
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	Fig. 3 Complete MIKE-echelle spectra of M 1-30.
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	Fig. 3 Complete MIKE-echelle spectra of M 1-32.
Open with DEXTER

	Fig. 3 Complete MIKE-echelle spectra of M 1-61.
Open with DEXTER

	Fig. 3 Complete MIKE-echelle spectra of M 3-15.
Open with DEXTER

	Fig. 3 Complete MIKE-echelle spectra of NGC 5189.
Open with DEXTER

	Fig. 3 Complete MIKE-echelle spectra of NGC 6369.
Open with DEXTER

	Fig. 3 Complete MIKE-echelle spectra of PC 14.
Open with DEXTER

	Fig. 3 Complete MIKE-echelle spectra of Pe 1-1.
Open with DEXTER

© ESO, 2012

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