Other
Scientific paper
Oct 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..20761085m&link_type=abstract
VizieR On-line Data Catalog: J/ApJS/76/1085. Originally published in: 1991ApJS...76.1085M
Other
Nebulae: Planetary, Magellanic Clouds, Spectroscopy
Scientific paper
We present optical spectroscopy in the range 3300-7400A for a total of 37 planetary nebulae in the LMC and seven in the SMC. Together with the object from the first paper in the series (1991ApJS...75..407M), we now have accurate emission-line intensities down to a few percent of Hβ for 77 nebulae in the Magellanic Clouds. Agreement with other authors is excellent. Reddening estimates from Balmer line ratios have been determined, and the line intensities have been dereddened accordingly. Nebular [O III] electron temperature and, where measurable, [S II] densities, are derived. [O II] electron densities are recalculated using appropriate electron temperatures. The [S II] and [O II] electron densities correlate well, with ne([O II])>ne([S II]). Zanstra temperatures are in derived for 22 objects possessing detectable stellar continua. These temperatures are in agreement with photoionization modeling of this sample. (1 data file).
Dopita Mike A.
Meatheringham Stephen J.
No associations
LandOfFree
LMC & SMC PNe optical spectroscopy. II (Meatheringham+ 1991) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with LMC & SMC PNe optical spectroscopy. II (Meatheringham+ 1991), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and LMC & SMC PNe optical spectroscopy. II (Meatheringham+ 1991) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1144365