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Gas dynamics and star formation in “isolated” and interacting galaxies using FP observations

Published online by Cambridge University Press:  14 May 2020

Isaura Fuentes-Carrera
Affiliation:
Escuela Superior de F sica y Matemáticas, Instituto Politécnico Nacional, (ESFM-IPN) U.P. Adolfo López Mateos, edifico 9, Zacatenco 07730, Mexico City, Mexico emails: ncardenas@esfm.ipn.mx, isaura@esfm.ipn.mx
Nelli Cárdenas-Martínez
Affiliation:
Escuela Superior de F sica y Matemáticas, Instituto Politécnico Nacional, (ESFM-IPN) U.P. Adolfo López Mateos, edifico 9, Zacatenco 07730, Mexico City, Mexico emails: ncardenas@esfm.ipn.mx, isaura@esfm.ipn.mx
Martín Nava-Callejas
Affiliation:
Escuela Superior de F sica y Matemáticas, Instituto Politécnico Nacional, (ESFM-IPN) U.P. Adolfo López Mateos, edifico 9, Zacatenco 07730, Mexico City, Mexico emails: ncardenas@esfm.ipn.mx, isaura@esfm.ipn.mx Instituto de Astronom a, Universidad Nacional Autónoma de México (UNAM) Apdo. Postal 70-264, 04510 Mexico City, Mexico emails: mnava@astro.unam.mx, margarit@astro.unam.mx
Margarita Rosado
Affiliation:
Instituto de Astronom a, Universidad Nacional Autónoma de México (UNAM) Apdo. Postal 70-264, 04510 Mexico City, Mexico emails: mnava@astro.unam.mx, margarit@astro.unam.mx
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Abstract

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We present scanning Fabry-Perot observations of different types of star-forming galaxies from apparently isolated LIRGs to equal mass interacting galaxies. We analyze the ionized gas kinematics, its relation with the morphology of each system and the location of SF regions for different systems.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

Footnotes

I.F.-C. thanks IPN project 20194926

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