Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/6545
Title: | Stellar Populations in the Magellanic Clouds |
Authors: | Smitha, S |
Issue Date: | Aug-2011 |
Publisher: | Indian Institute of Astrophysics |
Citation: | Ph.D. Thesis, Calicut University, Calicut |
Abstract: | The Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC) are two nearby galaxies located at a distance of 50 kpc and 60 kpc respectively. The Magellanic Clouds (MCs) host young, intermediate-age and old stellar populations. In this study, the stellar populations in the MCs are used as a tool to understand the structure and evolution of these galaxies as well as to understand the evolution of the Magellanic system as a whole. The structure of the MCs are studied using stellar populations (standard candles) of different ages (Cepheids - 100 Myr, Red clump stars: 2-9 Gyr & RR Lyrae stars > 9 Gyr) and the quantitative estimates of the structural parameters are derived. This study reveals the structural changes in the two galaxies as a function of time, and help to identify processes like interactions as well as mergers experienced by MCs at different epochs. |
Description: | Thesis Supervisor Dr.Annapurni Subramaniam |
URI: | http://hdl.handle.net/2248/6545 |
Appears in Collections: | IIAP Ph.D.Theses |
Files in This Item:
File | Description | Size | Format | |
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Stellar Populations in the Magellanic Clouds.pdf | 6.22 MB | Adobe PDF | View/Open |
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