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Key dynamical results from the SAMI Galaxy Survey

Published online by Cambridge University Press:  14 May 2020

Jesse van de Sande Open the ORCID record for Jesse van de Sande [Opens in a new window] ,
Joss Bland-Hawthorn ,
Dilyar Barat Open the ORCID record for Dilyar Barat [Opens in a new window] ,
Sarah Brough ,
Julia J. Bryant ,
Scott M. Croom ,
Luca Cortese  and
the SAMI Galaxy Survey collaboration
Jesse van de Sande
Affiliation:
Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW, 2006, Australia email: [email protected] ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia
Joss Bland-Hawthorn
Affiliation:
Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW, 2006, Australia email: [email protected] ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia
Dilyar Barat
Affiliation:
ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia Research School of Astronomy and Astrophysics, Australian National University, Canberra ACT 2611, Australia
Sarah Brough
Affiliation:
ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia School of Physics, University of New South Wales, NSW 2052, Australia
Julia J. Bryant
Affiliation:
Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW, 2006, Australia email: [email protected] ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia Australian Astronomical Optics, AAO-USydney, School of Physics, University of Sydney, NSW 2006, Australia
Scott M. Croom
Affiliation:
Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW, 2006, Australia email: [email protected] ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia
Luca Cortese
Affiliation:
ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia International Centre for Radio Astronomy Research, The University of Western Australia, 35 Stirling Highway, CrawleyWA6009, Australia
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Abstract

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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.

Keywords

galaxies: evolutiongalaxies: kinematics and dynamicsgalaxies: stellar content
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S353: Galactic Dynamics in the Era of Large Surveys , June 2019 , pp. 213 - 221
Copyright
© International Astronomical Union 2020

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