Optical spectroscopy of Magellanic Cloud planetary nebulae. III

Details Optical spectroscopy of Magellanic Cloud planetary nebulae. III Optical spectroscopy of Magellanic Cloud planetary nebulae. III

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apjs...83...87v&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 83, no. 1, p. 87-109.

Other

47

Balmer Series, Emission Spectra, Magellanic Clouds, Planetary Nebulae, Visible Spectrum, H Ii Regions, Hertzsprung-Russell Diagram, Photoionization, Stellar Spectrophotometry

Scientific paper

We present optical spectroscopy in the range 3400-7900 A for a total of 52 planetary nebulae (PNe) in the Large Magellanic Cloud (LMC) and 18 in the Small Magellanic Cloud (SMC). We have emission-line intensities for a total of 147 nebulae in the Magellanic Clouds. This sample contains a large selection of objects of low luminosity, with measurements of line intensities down to about 10 percent of Hβ. Brighter objects have line intensities measured down to around two percent of Hβ. Agreement with other derivations is generally very good. Reddening estimates from Balmer line ratios are determined: unreddened and reddened line intensities are tabulated.

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