Research Division Seminar
Unveiling the evolutionary history of the Magellanic Clouds through detection and analysis of stellar over-densities: clusters and streams.

Abstract

The Magellanic Clouds (MCs) are the closest example of a three-body
interacting system composed of the Milky Way (MW), the Large Magellanic Cloud
(LMC), and the Small Magellanic Cloud (SMC). Therefore, the unique opportunity
provided by their relative proximity allowed us to analyse with matchless detail
the dynamical and morphological evolution that a galaxy experience as a
consequence of the mutual gravitational interaction with its neighbors. In this
context, we performed a multi-faceted analysis, taking advantage of astrometric,
kinematics, and photometric data, with the main goal of unveiling the past
evolutionary path of the MCs and their intense interaction history. We tackled
this task by using two complementary approaches: (i) we adopted the properties
of the MCs star cluster (SC) system to get insights into their past evolution
and (ii) we probed the low-luminous regime of the outer regions of the MCs as
they are the most sensitive to recent or past tidal stripping events. I will
discuss the main outcomes up-to-date of this project and its future perspectives
in light of the new ongoing facilities.

Zoom link: https://rediris.zoom.us/j/81617686828?pwd=YUpBMXpobUpnYzlpUzluTGo1N2hRQT09

Meeing ID: 816 1768 6828

 Passcode: 990310

https://youtu.be/q1b98yBliFQ