Companions' influence on the emission-line rotation curves of galaxies

Details Companions' influence on the emission-line rotation curves of galaxies Companions' influence on the emission-line rotation curves of galaxies

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.191...49r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 191, no. 1, May 1992, p. 49-60.

Astronomy and Astrophysics

Astrophysics

2

Angular Velocity, Emission Spectra, Galactic Rotation, Interacting Galaxies, Line Spectra, Astronomical Catalogs, Correlation Coefficients

Scientific paper

The sample of members of isolated pairs of galaxies and close binary interacting systems - demonstrating a systematic falling of the emission-line rotation curves after the maxima - are considered. It is found that there is a significant correlation between the characteristics of the galaxies' emission-line velocity fields and the spatial distance to the companion. The different factors affecting the investigated relationships are discussed.

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