Physical characteristics of ionized gaseous nebulae

Details Physical characteristics of ionized gaseous nebulae Physical characteristics of ionized gaseous nebulae

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980srst.coll...99o&link_type=abstract

In NASA. Marshall Space Flight Center Sci. Res. with the Space Telescope p 99-121 (SEE N80-22130 12-88)

Astronomy and Astrophysics

Astronomy

3

Hubble Space Telescope, Ionized Gases, Nebulae, Spectroscopic Analysis, H Lines, Infrared Astronomy, Spectrum Analysis, Supernova Remnants, X Ray Astronomy

Scientific paper

The high angular resolution and the capability of the space telescope to observe ultraviolet radiation are discussed in relation to investigating planetary nebulae. The physical characteristics of planetary nebulae particulary the abundances of the common light elements, the H2 regions, the angular size, and the surface brightness are reviewed. Differences between supernova remants and planetary nebulae and H2 regions are discussed.

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