Spaxel analysis: Probing the physics of star formation in ultraluminous infrared galaxies
This paper presents a detailed spectral pixel (spaxel) analysis of the ten Luminous Infrared Galaxies (LIRGs) previously observed with the Wide Field Spectrograph (WiFeS), an integral field spectrograph mounted on the ANU 2.3 m telescope, and for which an abundance gradient analysis has already been presented by Rich et al. (Astrophys. J., 753:5, 2012). Here we use the strong emission line analysis techniques developed by Dopita et al. (Astrophys. J. Suppl. Ser., accepted, 2013) to measure the...[Show more]
|Collections||ANU Research Publications|
|Source:||Astrophysics and Space Science|
|01_Dopita_Spaxel_analysis:_Probing_the_2014.pdf||6.45 MB||Adobe PDF||Request a copy|
|02_Dopita_Spaxel_analysis:_Probing_the_2014.pdf||103.27 kB||Adobe PDF||Request a copy|
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