The dynamics of a giant filamentary shell in the LMC - II
Open Access
- 1 September 1980
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 192 (2) , 101-108
- https://doi.org/10.1093/mnras/192.2.101
Abstract
Profiles of the [O II] emission lines have been obtained at many positions over the giant filamentary shell, N70, in the LMC. Also a profile of the Ca II (K) interstellar absorption line was observed in the light of a centrally located OB star. Complex motions over a range of heliocentric radial velocities from 238 to 343 km s−1 have been discovered which could be explained by separate expanding shells in both of the large clouds of neutral hydrogen (McGee & Milton 1966) in this vicinity.Keywords
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