# name
Chemo-kinematic characterisation of the Red Clump stars of the Galactic bar

# metadata.dc.description[].value
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutora: Mercè Romero Gómez

# metadata.dc.description.abstract[].value
Thanks to recent surveys, we now have larger homogeneous data sets containing kinematics and metallicities of stars outside the solar neighbourhood. From a cross-match between Gaia DR2 and APOGEE DR16 data, we can study the complex chemical and dynamical structure of the galactic disk, which is perturbed by the existence of a galactic bar. We run an orbital integrator to classify the 3D quasiperiodic orbits into the diﬀerent resonant families. Since the cross-match between GAIA DR2 and APOGEE DR16 data gives us also the metallicities, we then investigate the eﬀect of bar resonances on the metallicity distribution in the Milky Way

# metadata.dc.title[].value
Chemo-kinematic characterisation of the Red Clump stars of the Galactic bar