The nature of the core of the 30 Doradus Nebula from new optical observations

Details The nature of the core of the 30 Doradus Nebula from new optical observations The nature of the core of the 30 Doradus Nebula from new optical observations

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....84..167c&link_type=abstract

Astronomy and Astrophysics, vol. 84, no. 1-2, Apr. 1980, p. 167-176. Research supported by the Science Research Council.

Astronomy and Astrophysics

Astrophysics

25

Nebulae, Optical Emission Spectroscopy, Spectrum Analysis, Visual Observation, Angular Resolution, Astronomical Photography, Cores, Density Measurement, Magellanic Clouds, Radial Velocity, Telescopes, Velocity Measurement

Scientific paper

A variety of new optical observations have been made, with advanced instruments, of the bright core of the 30 Doradus Nebula.
Velocity and density measurements from emission and absorption lines have been made at unprecedented angular and wavelength resolutions, and signal to noise ratios, with 1.9-m and 3.9-m telescopes. Furthermore, filter photographs have been printed through unsharp masks. Many new and unusual aspects of the nature of this complex region are revealed.

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