Spectrophotometry of four galaxies of high surface brightness

Details Spectrophotometry of four galaxies of high surface brightness Spectrophotometry of four galaxies of high surface brightness

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..334a&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, June 1982, p. 334-338.) Soviet Astronomy Letters, vol. 8, May-June 1982, p. 181-183.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Emission Spectra, Galactic Radiation, Spectrophotometry, Galactic Nuclei, Hydrogen Clouds, Spectral Line Width

Scientific paper

Spectrophotometry has been performed for the emission lines in the
nuclei of Arakelian galaxies nos. 428, 449, 454, 532. In the first two
objects, H II clouds occur approximately 2 kpc out from the nucleus. No.
449 may contain another cloud moving at approximately 1500 km/sec radial
velocity.

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