Inhomogeneities in the Bubble nebula, NGC 7635

Details Inhomogeneities in the Bubble nebula, NGC 7635 Inhomogeneities in the Bubble nebula, NGC 7635

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...274..650l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 274, Nov. 15, 1983, p. 650-658.

Astronomy and Astrophysics

Astrophysics

10

Abundance, Emission Spectra, Hydrogen Clouds, Molecular Clouds, Nebulae, Electron Density (Concentration), Forbidden Bands, H Alpha Line, Radial Velocity

Scientific paper

Intensities of select emission lines of H, He I, and the forbidden lines N II, O III, O II, and S II are measured in sample regions within NGC 7635. Several bright knots are interpreted as emission rims of globules. The Bubble appears to be a unique region characterized by enhanced forbidden line O III and lower fractions of the N II and S II forbidden lines. The nebula may be interpreted as a dusty blister on the edge of a molecular cloud.

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