TY - JOUR
T1 - Key dynamical results from the SAMI Galaxy Survey
AU - Van De Sande, Jesse
AU - Bland-Hawthorn, Joss
AU - Barat, Dilyar
AU - Brough, Sarah
AU - Bryant, Julia J.
AU - Croom, Scott M.
AU - Cortese, Luca
N1 - Publisher Copyright:
© 2020 International Astronomical Union.
PY - 2019
Y1 - 2019
N2 - We present an overview of recent key results from the SAMI Galaxy Survey on the build-up of mass and angular momentum in galaxies across morphology and environment. The SAMI Galaxy survey is a multi-object integral field spectroscopic survey and provides a wealth of spatially-resolved, two-dimensional stellar and gas measurements for galaxies of all morphological types, with high-precision due the stable spectral resolution of the AAOmega spectrograph. The sample size of ∼3000 galaxies allows for dividing the sample in bins of stellar mass, environment, and star-formation or morphology, whilst maintaining a statistical significant number of galaxies in each bin. By combining imaging, spatially resolved dynamics, and stellar population measurements, our result demonstrate the power of utilising integral field spectroscopy on a large sample of galaxies to further our understanding of physical processes involved in the build-up of stellar mass and angular momentum in galaxies.
AB - We present an overview of recent key results from the SAMI Galaxy Survey on the build-up of mass and angular momentum in galaxies across morphology and environment. The SAMI Galaxy survey is a multi-object integral field spectroscopic survey and provides a wealth of spatially-resolved, two-dimensional stellar and gas measurements for galaxies of all morphological types, with high-precision due the stable spectral resolution of the AAOmega spectrograph. The sample size of ∼3000 galaxies allows for dividing the sample in bins of stellar mass, environment, and star-formation or morphology, whilst maintaining a statistical significant number of galaxies in each bin. By combining imaging, spatially resolved dynamics, and stellar population measurements, our result demonstrate the power of utilising integral field spectroscopy on a large sample of galaxies to further our understanding of physical processes involved in the build-up of stellar mass and angular momentum in galaxies.
KW - galaxies: evolution
KW - galaxies: kinematics and dynamics
KW - galaxies: stellar content
UR - http://www.scopus.com/inward/record.url?scp=85085062155&partnerID=8YFLogxK
U2 - 10.1017/S174392131900913X
DO - 10.1017/S174392131900913X
M3 - Review article
SN - 1743-9213
VL - 14
SP - 213
EP - 221
JO - Proceedings of the International Astronomical Union
JF - Proceedings of the International Astronomical Union
IS - S353
ER -