Rotation curves in (E+S) isolated galaxy pairs

Details Rotation curves in (E+S) isolated galaxy pairs Rotation curves in (E+S) isolated galaxy pairs

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009rmxac..35..227h&link_type=abstract

XII Latin American IAU Regional Meeting (Eds. G. Magris, G. Bruzual, & L. Carigi) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Galaxies: Kinematics And Dynamics

Scientific paper

As part of a broad investigation to quantify the effects of interaction in the evolution of disk galaxies, we measured rotation curves of 102 spirals in mixed morphology pairs (E+S), drawn from the Karachantsev catalogue of isolated pairs of galaxies. In this summary we simply present characteristic rotation curves of spirals in isolated (E+S) pairs, in preparation for a future comparison with isolated spirals in a Tully-Fisher diagram.

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