A spectroscopic study of the multicomponent interacting system of galaxies VV 126

Details A spectroscopic study of the multicomponent interacting system of galaxies VV 126 A spectroscopic study of the multicomponent interacting system of galaxies VV 126

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980sval....6..110m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Apr. 1980, p. 202-207.) Soviet Astronomy Letters, vol. 6, Mar.-Apr. 1980, p. 110-113

Astronomy and Astrophysics

Astronomy

1

Astronomical Spectroscopy, Galaxies, Interacting Galaxies, Emission Spectra, H Ii Regions, Hydrogen Ions, Line Spectra, Spectrograms, Velocity Distribution

Scientific paper

VV 126 has been investigated on spectrograms taken with the 6-m telescope. This object is a system of two or more distorted giant galaxies having a peculiar velocity field and emission knots representing giant H II regions, or superassociations. If the system is stable its total mass should be equal to about 10 to the 11th solar masses. The relative emission-line intensities are similar to those observed for H II regions in the spiral structure of ordinary galaxies.

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