The dynamics of the giant filamentary shell, N 51 D, in the LMC

Details The dynamics of the giant filamentary shell, N 51 D, in the LMC The dynamics of the giant filamentary shell, N 51 D, in the LMC

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....89..126m&link_type=abstract

Astronomy and Astrophysics, vol. 89, no. 1-2, Sept. 1980, p. 126-131. Research sponsored by the Science Research Council.

Astronomy and Astrophysics

Astrophysics

26

Astronomical Spectroscopy, Magellanic Clouds, Nebulae, Emission Spectra, Forbidden Bands, Line Spectra, Stellar Winds, Supernova Remnants

Scientific paper

The profiles of the forbidden O II emission lines have been observed at
many positions over the giant filamentary shell N 51 D. Evidence is
presented which suggests that this nebula could either be an expanding
spherical shell driven by energetic stellar winds or more likely a
supernova remnant approaching fossilization.

Affiliated with

Also associated with

No associations

Rating

The dynamics of the giant filamentary shell, N 51 D, in the LMC 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 The dynamics of the giant filamentary shell, N 51 D, in the LMC, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The dynamics of the giant filamentary shell, N 51 D, in the LMC will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-903671