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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: [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.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

Footnotes

I.F.-C. thanks IPN project 20194926

References

Arp, H. 1966, ApJS, 14, 110.1086/190147CrossRefGoogle Scholar
Bell, E. F., Papovich, C., Wolf, C., Le Floc’h, E., Caldwemm, J. A. R., & 9 co-authors 2005. ApJ, 625, 2310.1086/429552CrossRefGoogle Scholar
Cárdenas-Mart nez , N. & Fuentes-Carrera, I. 2018, ApJ, 868, 14110.3847/1538-4357/aae891CrossRefGoogle Scholar
Fuentes-Carrera, I., Rosado, M., Amram, P., Laurikainen, E., Salo, H., Gómez-López, J. A., Castañeda, H. O., Bernal, A., & Balkowski, C. 2019, A&A, 621A, 25Google Scholar
Krabbe, A. C., Rosa, D. A., Pastoriza, M. G., et al. 2017, MNRAS, 467, 2710.1093/mnras/stw3128CrossRefGoogle Scholar
Larson, K. L., Sanders, D. B., Barnes, J. E., Ishida, C. M., Evans, A. S., U, V., Mazzarella, J. M., Kim, D.-C., Privon, G. C., Mirabel, I. F., & Flewelling, H. A 2016, ApJ, 825, 12810.3847/0004-637X/825/2/128CrossRefGoogle Scholar
Lotz, J. M., Davis, M., Faber, S. M., Guhathakurta, P., Gwyn, S., Huang, J., Koo, D. C., & 14 co-authors 2008. ApJ, 672, 17710.1086/523659CrossRefGoogle Scholar
Rosado, M., Langarica, R., Bernal, A., et al. 1995, RMxAC, 3, 263Google Scholar
Schreiber, C., Pannella, M., Elbaz, D., et al. 2015, A&A, 575, A74Google Scholar