Galactic Line Emission

Research on the photo-excited component of the interstellar medium continues through our involvement with various large scale surveys of the Galactic Plane. These surveys have included the Southern H-alpha Survey and its northern sky counterpart IPHAS. More recently we have been using high quality data of the Southern Milky Way from VPHAS+ and we will be returning to the Northern Sky using data from the WEAVE project.

Supernova remnant S147 in H-alpha. Created by Nick Wright of Keele University using data from the IPHAS project
A 5°×3.5° mosaic of the supernova remnant S147 in Hα. North is to the top and East to the left. Image credit: Nick Wright of Keele University using data from the IPHAS project.
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