The past, present and future of Galactic planetary nebula surveys

TL;DR

Recent advances in high-sensitivity, multi-wavelength surveys have revolutionized the discovery and understanding of Galactic planetary nebulae, revealing new insights into late-stage stellar evolution.

Contribution

This review synthesizes recent survey developments, contextualizes past progress, and discusses future opportunities in Galactic planetary nebula research.

Findings

Increased discovery rate of planetary nebulae.

Enhanced diagnostic capabilities from multi-wavelength data.

Realization of astrophysical potential of late-stage stellar evolution.

Abstract

Over the last decade Galactic planetary nebula discoveries have entered a golden age due to the emergence of high sensitivity, high resolution narrow-band surveys of the Galactic plane. These have been coupled with access to complimentary, deep, multi-wavelength surveys across near-IR, mid-IR and radio regimes in particular from both ground-based and space-based telescopes. These have provided powerful diagnostic and discovery capabilities. In this review these advances are put in the context of what has gone before, what we are uncovering now and through the window of opportunity that awaits in the future. The astrophysical potential of this brief but key phase of late stage stellar evolution is finally being realised.