Galactic ring nebulae associated with Wolf-Rayet stars. III - H II region-type nebulae

Details Galactic ring nebulae associated with Wolf-Rayet stars. III - H II region-type nebulae Galactic ring nebulae associated with Wolf-Rayet stars. III - H II region-type nebulae

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...250..615c&link_type=abstract

Astrophysical Journal, Part 1, vol. 250, Nov. 15, 1981, p. 615-620.

Astronomy and Astrophysics

Astrophysics

27

Astronomical Spectroscopy, H Ii Regions, Interstellar Matter, Line Spectra, Nebulae, Wolf-Rayet Stars, Emission Spectra, Fabry-Perot Interferometers, Ring Structures, Stellar Winds

Scientific paper

Fabry-Perot data for five galactic ring nebulae associated with Wolf-Rayet stars have been obtained. The amount of turbulence in these nebulae is comparable to that in an ordinary H II region. It seems that these nebulae are only being illuminated by the central star. There is no evidence that these nebulae are formed from either material ejected from the stars or by stellar winds interacting with the interstellar medium.

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