Rotation curves in (E+S) isolated galaxy pairs
Por:
Huerta E.M., González J.J.
Publicada:
1 ene 2009
Resumen:
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.
Filiaciones:
Huerta E.M.:
Centro de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de Méxiso, Apdo. Postal 3-72, 58090, Morelia, Michoacán, Mexico
González J.J.:
Instituto de Astronomía, Universidad Nacional Autónoma de Méxiso, Apdo. Postal 70-264, 04510, Méxiso D.F., Mexico
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