Mapping electron temperature variations across a spiral arm in NGC 1672

I-Ting Ho, Kathryn Kreckel, Sharon E. Meidt, Brent Groves, Guillermo A. Blanc, Frank Bigiel, Daniel A. Dale, Eric Emsellem, Simon C. O. Glover, Kathryn Grasha, Lisa J. Kewley, J. M. Diederik Kruijssen, Philipp Lang, Rebecca McElroy, Rolf-Peter Kudritzki, Patricia Sanchez-Blazquez, Karin Sandstrom, Francesco Santoro, Eva Schinnerer, Andreas Schruba

Published 2019-10-22Version 1

We report one of the first extragalactic observations of electron temperature variations across a spiral arm. Using MUSE mosaic observations of the nearby galaxy NGC 1672, we measure the [N II]5755 auroral line in a sample of 80 HII regions in the eastern spiral arm of NGC1672. We discover systematic temperature variations as a function of distance perpendicular to the spiral arm. The electron temperature is lowest on the spiral arm itself and highest on the downstream side. Photoionization models of different metallicity, pressure, and age of the ionizing source are explored to understand what properties of the interstellar medium drive the observed temperature variations. An azimuthally varying metallicity appears to be the most likely cause of the temperature variations. The electron temperature measurements solidify recent discoveries of azimuthal variations of oxygen abundance based on strong lines, and rule out the possibility that the abundance variations are artefacts of the strong-line calibrations.