A radio-optical study of resolved star formation in SAMI galaxies
With integral field spectroscopic data from the the Sydney-AAO Multi-object Integralfield spectrograph (SAMI) survey and the VLA, we will study the relationship between star formation (as traced by H innodataalpha emission) and the radio continuum emission within galaxies with the aim of better understanding the intricacies of local scaling relations.
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|Source:||International Astronomical Union. Proceedings|
|01_Leslie_A_radio-optical_study_of_2014.pdf||39.62 kB||Adobe PDF||Request a copy|
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