The dynamics and structure of the ionized and neutral gas in the 30 Doradus nebula

Details The dynamics and structure of the ionized and neutral gas in the 30 Doradus nebula The dynamics and structure of the ionized and neutral gas in the 30 Doradus nebula

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..78..443w&link_type=abstract

Astrophysics and Space Science, vol. 78, no. 2, Aug. 1981, p. 443-461. Research supported by the Science Research Council.

Astronomy and Astrophysics

Astrophysics

7

Gas Dynamics, Nebulae, Neutral Gases, Absorption Spectra, Astronomical Photography, Gas Density, H Ii Regions, Propagation Velocity, Radial Velocity

Scientific paper

A variety of new optical observations have been made over the bright core of the supermassive H II region 30 Doradus and the ionized filamentary material surrounding this object. In addition, a more detailed analysis of previously published interstellar absorption and H I emission profiles has been undertaken. The velocity and density structure of this complex region is discussed and the new results analyzed here shown to be compatible to the model of 30 Doradus presented in Canto et al. (1980) and Meaburn (1980).

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