Effect of the gas percentage on the thickness of the galactic discs during minor mergers using hydrodynamical simulations
| Autor: | S. N. Hasan, Swetha Thakkalapally, Priya Hasan |
|---|---|
| Rok vydání: | 2019 |
| Předmět: |
Physics
Mathematics::Complex Variables Space and Planetary Science Primary (astronomy) Minor (linear algebra) Astronomy and Astrophysics Astrophysics::Earth and Planetary Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Mass ratio Disc galaxy Astrophysics::Galaxy Astrophysics Galaxy |
| Zdroj: | Proceedings of the International Astronomical Union. 14:281-283 |
| ISSN: | 1743-9221 1743-9213 |
| DOI: | 10.1017/s174392131900824x |
| Popis: | We study the minor mergers of galaxies using simulations. For this we use GADGET2 code. We present results of simulations of minor mergers of disc galaxies of mass ratio 1:10. These simulations consist of collisionless as well as hydrodynamical runs including a gaseous component in the galactic disc of primary galaxy. Our goal is to establish the characteristics of discs obtained after the merger.We observe that the primary galaxy discs are not destroyed after the merger. We take different initial conditions for the primary galaxy varying the gas percentage in disc from 0–40 percentage and study the thickness of the disc after the merger. We generally observe that the thickness of the disc increases after the merger for any gas percentage. We also observe that as the gas percentage increases in the disc of initial primary galaxy, the increase in the thickness keeps decreasing. |
| Databáze: | OpenAIRE |
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