Spectrophotometry of Selected Planetary Nebulae of Type I in the Magellanic Clouds

Details Spectrophotometry of Selected Planetary Nebulae of Type I in the Magellanic Clouds Spectrophotometry of Selected Planetary Nebulae of Type I in the Magellanic Clouds

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...180.3913t&link_type=abstract

American Astronomical Society, 180th AAS Meeting, #39.13; Bulletin of the American Astronomical Society, Vol. 24, p.792

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Scientific paper

We present observations carried out with the CTIO 4-m telescope of the planetary nebulae: N 67, in the Small Magellanic Cloud, N 66, N 97, and N 102 in the Large Magellanic Cloud. They are among the brightest PN in the Magellanic Clouds and have been extensively studied by other authors. We derive their physical conditions and chemical compositions. These objects are of high electron density and high electron temperature, which makes them excellent probes to study collisional effects on the He I lines, and in particular, the population of the 2(3) S level of He I.

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