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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 Open the ORCID record for Isaura Fuentes-Carrera [Opens in a new window] ,
Nelli Cárdenas-Martínez ,
Martín Nava-Callejas  and
Margarita Rosado
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: [email protected], [email protected]
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: [email protected], [email protected]
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: [email protected], [email protected] Instituto de Astronom a, Universidad Nacional Autónoma de México (UNAM) Apdo. Postal 70-264, 04510 Mexico City, Mexico emails: [email protected], [email protected]
Margarita Rosado
Affiliation:
Instituto de Astronom a, Universidad Nacional Autónoma de México (UNAM) Apdo. Postal 70-264, 04510 Mexico City, Mexico emails: [email protected], [email protected]
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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.

Keywords

galaxies: interactionsgalaxies: kinematics and dynamicsgalaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S353: Galactic Dynamics in the Era of Large Surveys , June 2019 , pp. 264 - 265
Copyright
© International Astronomical Union 2020

Footnotes

†

I.F.-C. thanks IPN project 20194926

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