Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.238...67v&link_type=abstract
Astrophysics and Space Science, Volume 238, Issue 1, pp.67-70
Astronomy and Astrophysics
Astrophysics
2
Uv Spectroscopy, Stellar Winds, Magellanic Clouds, Planetary Nebula Nuclei
Scientific paper
Narrow-band [O III] 500.7 nm images and ultraviolet spectrophotometry are obtained for ≈20 planetary nebulae (PNe) in the Magellanic Clouds using the Hubble Space Telescope (HST). Four objects show P Cygni-like features in the ultraviolet HST data, and/or broad emission complexes near the He II 468.6 nm and C IV 580.6 nm lines in ground-based spectra. All objects are of excitation class four or lower, and all are compact and dense compared to other objects in the sample. The likelihood of detecting ultraviolet P Cygni-like profiles in future HST spectroscopy of other objects is discussed.
No associations
LandOfFree
Hubble Space Telescope observations of Magellanic cloud planetary nebulae: Stellar winds 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 Hubble Space Telescope observations of Magellanic cloud planetary nebulae: Stellar winds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hubble Space Telescope observations of Magellanic cloud planetary nebulae: Stellar winds will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1333964