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

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