Spectrophotometric Study of Galaxies with UV Excess

Details Spectrophotometric Study of Galaxies with UV Excess Spectrophotometric Study of Galaxies with UV Excess

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap.....47...65k&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 47, Issue 1, p. 65-71 (2004).

Astronomy and Astrophysics

Astrophysics

Galaxies - Galaxies Spectrophotometry

Scientific paper

Results from a spectrophotometric study of 21 galaxies with UV excess are presented. The half widths (FWHM) and equivalent widths of observed spectrum lines of these galaxies, as well as the relative intensities of the emission lines observed in the spectrum of the galaxy Kaz243, are determined. It is conjectured that the latter galaxy has the properties of an Sy2 type galaxy. The electron densities and masses of the gaseous components are found for 15 galaxies, along with the masses of 8 galaxies for which the ratio M/L has been calculated. It is shown that the spectral structures of these galaxies do not depend on whether they are members of physical systems or are isolated.

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