H I, molecular/H II shells from 1 to 2000 PC diameter - Wind-driven or supernova remnants

Details H I, molecular/H II shells from 1 to 2000 PC diameter - Wind-driven or supernova remnants H I, molecular/H II shells from 1 to 2000 PC diameter - Wind-driven or supernova remnants

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..59..193m&link_type=abstract

Astrophysics and Space Science, vol. 59, no. 1, Nov. 1978, p. 193-214. Research sponsored by the Science Research Council.

Astronomy and Astrophysics

Astronomy

30

Hydrogen Clouds, Stellar Winds, Supernova Remnants, H Lines, Nebulae, Ultraviolet Astronomy

Scientific paper

Deep H-alpha + forbidden N II photographs of five giant shell-like nebulas in the LMC are compared to 21-cm H I maps, Schmidt photographs showing the O and B associations and the UV sources from 1200 to 1600 A. The formation of all shell-like nebulas which do not appear to be supernova remnants and which have diameters between 1 pc and 1900 pc is discussed.

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