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A Radio-Optical Study of Resolved Star Formation in SAMI Galaxies

Published online by Cambridge University Press:  09 February 2015

Sarah Leslie ,
Lisa Kewley ,
Elaine Sadler  and
Julia Bryant
Sarah Leslie
Affiliation:
School of Astronomy & Astrophysics, Australian National University, Cotter Road, Weston, ACT 2611, Australia email: u5022102@anu.edu.au ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)
Lisa Kewley
Affiliation:
School of Astronomy & Astrophysics, Australian National University, Cotter Road, Weston, ACT 2611, Australia email: u5022102@anu.edu.au
Elaine Sadler
Affiliation:
Sydney Institute for Astronomy (SIfA), School of Physics, The University of Sydney, NSW 2006, Australia ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)
Julia Bryant
Affiliation:
Sydney Institute for Astronomy (SIfA), School of Physics, The University of Sydney, NSW 2006, Australia ARC Centre of Excellence for All-sky Astrophysics (CAASTRO) The Australian Astronomical Observatory, PO Box 915, North Ryde, NSW, 1670, Australia
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Abstract

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With integral field spectroscopic data from the the Sydney-AAO Multi-object Integral-field spectrograph (SAMI) survey and the VLA, we will study the relationship between star formation (as traced by Hα emission) and the radio continuum emission within galaxies with the aim of better understanding the intricacies of local scaling relations.

Keywords

galaxies: star formationradio continuum: galaxiesgalaxies: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 324
Copyright
Copyright © International Astronomical Union 2015