Definition of "wim"

Confirming and strengthening our conclusions in Papaderos et al. (2013) we argue that ETGs span a broad continuous sequence with regard to the properties of their wim, and they can be roughly subdivided into two characteristic classes.

2015, J.M. Gomes, P. Papaderos, C. Kehrig, J.M. Vílchez, M.D. Lehnert, CALIFA collaboration, “Extended nebular emission in CALIFA early-type galaxies”, in arXiv‎