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The evolution of bulges of galaxies in minor fly-by interactions

Published online by Cambridge University Press:  14 May 2020

Ankit Kumar Open the ORCID record for Ankit Kumar [Opens in a new window] ,
Mousumi Das  and
Sandeep Kumar Kataria
Ankit Kumar
Affiliation:
Indian Institute of Astrophysics, Bengaluru, 560034, India email: [email protected] Department of physics, Indian Institute of Science, Bengaluru, 560012, India
Mousumi Das
Affiliation:
Indian Institute of Astrophysics, Bengaluru, 560034, India email: [email protected]
Sandeep Kumar Kataria
Affiliation:
Indian Institute of Astrophysics, Bengaluru, 560034, India email: [email protected] Department of physics, Indian Institute of Science, Bengaluru, 560012, India
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Abstract

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We investigate the minor interactions of two disk galaxies with mass ratio of 10:1 in fly-by encounters that do not lead to the merging of the galaxies. In our N-body simulations, we vary only the pericenter distances to see the effect of the fly-by on the bulge of the major galaxy over the course of the trajectory. At different time steps of the evolution, we did two-dimensional fittings of disk, bulge and bar to trace the variation in the sersic index of the bulge. Our results suggest that galaxy bulges can become boxy/disky through flyby interactions of galaxies.

Keywords

Methods: N-body simulationsGalaxies: BulgesGalaxies: Interactions
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. 166 - 167
Copyright
© International Astronomical Union 2020

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