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Emission-Line Diagnostics for Galaxies

Published online by Cambridge University Press:  27 October 2016

Lisa J. Kewley
Lisa J. Kewley*
Affiliation:
RSAA, Australian National University, Cotter Road, Weston Creek, ACT 2611, Australia Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI, USA email: kewley@mso.anu.edu.au
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Abstract

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I will give an overview of the emission-line diagnostics used for star-forming galaxies. I will review the UV, optical, and IR diagnostics that can be used to yield information about the ISM conditions, star-formation properties, and power sources in GRB hosts, both globally, and with spatially-resolved data. I will discuss wide integral field spectroscopy and AO-led integral field spectroscopy on current and future telescopes, focusing on the insights to be gained on the properties of GRB sites.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 264
Copyright
Copyright © International Astronomical Union 2016