IUE spectra of the nuclei of M31 and M32

Details IUE spectra of the nuclei of M31 and M32 IUE spectra of the nuclei of M31 and M32

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...230l.137j&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 230, June 15, 1979, p. L137-L140.

Astronomy and Astrophysics

Astronomy

33

Absorption Spectra, Galactic Nuclei, Iue, Satellite Observation, Spaceborne Astronomy, Ultraviolet Spectra, Andromeda Galaxy, Hot Stars, Nebulae, Quasars, Radiant Flux Density, Spectrophotometry

Scientific paper

Observed spectra are reproduced in the 1000-3400 wavelength range; line identifications are tabulated, and spectrophotometry of parts of the continua is given. The flux density of a few line emissions can be estimated from their equivalent widths. The strongest line emissions differ in the two nuclei, and they do not fit spectral patterns that are observed in the sun, hot stars, gaseous nebulae, or quasi-stellar objects. However, the absorption-line features are rather similar to those of the sun.

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