|
DSpace - Tor Vergata >
Facoltà di Scienze Matematiche Fisiche e Naturali >
Tesi di dottorato in scienze matematiche e fisiche >
Please use this identifier to cite or link to this item:
http://hdl.handle.net/2108/208
|
| Title: | Detailed chemical abundances in the Sgr and CMa dwarf galaxies |
| Authors: | Buonanno, Roberto Sbordone, Luca |
| Keywords: | abundances atmospheres dwarf evolution stellar content Sgr dSph |
| Issue Date: | 21-Feb-2006 |
| Abstract: | Abstract
Detailed chemical abundances for up to 23 elements from Oxygen to Europium have been obtained
from VLT-UVES spectra for 12 giants in the Sagittarius Dwarf Spheroidal galaxy (Sgr dSph), 5 in the
associated globular cluster Terzan 7, and 3 in the direction of the newly discovered and still controversial
CMa overdensity. The analysis has been accomplished by means of a GNU-Linux ported version of R.
L. Kurucz’s codes for atmosphere modeling (ATLAS), abundance determination (WIDTH) and spectral
synthesis (SYNTHE). The porting details are discussed in the thesis, the ported codes are freely available
on line.
Sgr dSph is the nearest confirmed dwarf spheroidal galaxy. Moving along a short period, quasi-polar
orbit around the Milky Way (MW) it is undergoing tidal disruption inside the Halo. It is, consequently,
an ideal test case for studying the role of tidal merging in shaping our Galaxy. In this study we evidence
the presence of a metal rich (from [Fe/H]» −0.8 up to sli... |
| URI: | http://hdl.handle.net/2108/208 |
| Appears in Collections: | Tesi di dottorato in scienze matematiche e fisiche
|
Files in This Item:
| File |
Description |
Size | Format |
| tesi_PhD.pdf | | 2239Kb | Adobe PDF | View/Open |
|
Show full item record
All items in DSpace are protected by copyright, with all rights reserved.
|