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http://hdl.handle.net/2248/6594| Title: | Stellar populations in the magellanic clouds |
| Authors: | Subramanian, S Subramaniam, A |
| Keywords: | Galaxies Magellanic Clouds Stars: Distances Stars: Horizontal Branch Stars: Variables Cepheids |
| Issue Date: | 2013 |
| Publisher: | Astronomical Society of India |
| Citation: | Khare, Pushpa and Ishwara-Chandra C.H., eds., Proceedings of the 31st meeting of the Astronomical Society of India, February 20-22, 2013 , pp. 63 - 66 |
| Series/Report no.: | Astronomical Society of India Conference Series;9 |
| Abstract: | The structural parameters of the Large Magellanic Cloud and the Small Magellanic Cloud are derived from the study of di erent stellar populations, such as, Cepheids (age 100 Myr), Red Clump stars (age 2-9 Gyr) and RR Lyrae stars (age > 9 Gyr). The structural changes of these galaxies as a function of time are identified and the processes which are responsible for these changes are discussed. The formation and early evolution of these two galaxies are found to be di erent. |
| Description: | Open Access |
| URI: | http://hdl.handle.net/2248/6594 |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Stellar populations in the magellanic clouds.pdf | Open Access | 114.95 kB | Adobe PDF |  View/Open |
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