Please use this identifier to cite or link to this item:
http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1673| Galaxy pairs in the galaxy and mass assembly (GAMA) survey: the interplay between galaxy mass, star formation rate and the heavy elements abundance | |
| LUIS ENRIQUE GARDUÑO PUGA | |
| Omar López Cruz MARITZA ARLENE LARA LOPEZ | |
| Acceso Abierto | |
| Atribución-NoComercial-SinDerivadas | |
| Galaxies Pairs Survey SFR Metallicity | |
| This project is focused on the analysis of galaxy pairs since they are the minimal unit in which changes of different properties can be measured, such as star formation rate and metallicity. Data are taken from the Galaxy and Mass Assembly Survey II (GAMAII). The 2dF robot positioner of fibres solved the problem of fiber collision (seen in SDSS), this makes the GAMA survey highly complete and ideal for the study of pairs and groups of galaxies. We selected galaxies at all multiplicities, with a maximum angular separation of 100 arcsec, relative velocity ∆𝜈 < 1000 km s⁻¹, S/N > 3 and a redshift interval | |
| Instituto Nacional de Astrofísica, Óptica y Electrónica. | |
| 2019-02 | |
| Tesis de maestría | |
| Inglés | |
| Estudiantes Investigadores Público en general | |
| Garduño Puga, L. E., (2019), Galaxy pairs in the galaxy and mass assembly (GAMA) survey: the interplay between galaxy mass, star formation rate and the heavy elements abundance, Tesis de Maestría, Instituto Nacional de Astrofísica, Óptica y Electrónica. | |
| ASTRONOMÍA Y ASTROFÍSICA | |
| Versión aceptada | |
| acceptedVersion - Versión aceptada | |
| Appears in Collections: | Maestría en Astrofísica |
Upload archives
| File | Size | Format | |
|---|---|---|---|
| GarduñoPLE.pdf | 9.78 MB | Adobe PDF | View/Open |