Hostname: page-component-848d4c4894-8bljj Total loading time: 0 Render date: 2024-06-27T18:37:44.444Z Has data issue: false hasContentIssue false

Kinematic properties of superbubbles in the Antennae, M83 and Arp 270

Published online by Cambridge University Press:  09 February 2015

A. Camps-Fariña
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain Departamento de Astrofísica, Universidad de la Laguna, Spain
J. Beckman
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain Departamento de Astrofísica, Universidad de la Laguna, Spain Consejo Superior de Investigaciones Científicas, Spain
J. Zaragoza-Cardiel
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain Departamento de Astrofísica, Universidad de la Laguna, Spain
J. Font
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain Departamento de Astrofísica, Universidad de la Laguna, Spain
K. Fathi
Affiliation:
Department of Astronomy, Stockholm University, Stockholm, Sweden
P. Fabian Velázquez
Affiliation:
Instituto de Ciencias Nucleares, Universidad Nacional de México, D.F, Mexico
A. Rodríguez-González
Affiliation:
Instituto de Ciencias Nucleares, Universidad Nacional de México, D.F, Mexico
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Superbubbles and large scale expansion in galaxies are important indicators of activity in galaxies: they are formed in starbursts and around active nuclei. Superbubbles can be used to give information about the star-forming region which produced them. We present in-depth results of our study of kinematically detected superbubbles using a method based on Fabry-Perot spectroscopy, which allows us to map regions of expansion across the entire disk of a galaxy. Three objects have been selected for this poster based on the interest of the results they show: two interacting galaxies, the Antennae and Arp270, at different stages of galaxy interaction, and the more isolated galaxy M83. We present the kinematic expansion maps, as well as a census of detected superbubbles and a dynamical study of their properties.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Raga, A. C., Navarro-González, R., & Villagrán-Muniz, M., 2000, RMxAA, 36, 67Google Scholar