Complex and broad H I profiles in the vicinity of giant LMC shells

Details Complex and broad H I profiles in the vicinity of giant LMC shells Complex and broad H I profiles in the vicinity of giant LMC shells

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.206..705m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 206, Feb. 15, 1984, p. 705-711.

Astronomy and Astrophysics

Astronomy

25

Hydrogen Clouds, Magellanic Clouds, Nebulae, Neutral Gases, Radial Velocity, Radio Sources (Astronomy), B Stars, Centimeter Waves, H Lines, O Stars, Stellar Envelopes

Scientific paper

Profiles of the 21-cm line from H I have been obtained both on and off 11 of the giant interstellar shells in the Large Magellanic Cloud. Separate velocity components over a range of heliocentric radial velocity of 142 - 380 km s-1 have been found over an area ⪆490 pc across in the vicinity of N185 and N186. No evidence is found in these profiles for internally generated motions of the neutral material in any of the shells, although many new velocity components have been discovered.

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