arXiv2001
We report the discovery of a extremely narrow, extremely linear, ionized filament. The filament is 2.5 degrees long and has an H$α$ surface brightness of 0.5 rayleighs. The filament is approximately ``Y'' shaped. The widest separation of the two diagonal segments is 5 arcminutes. We discuss four possible origins for this feature: (1) an extremely low density, nearby jet, (2) an unusually linear filament associated with some large-scale nearby nebula, perhaps even the Local Bubble, (3) an ionized trail left by mechanical input from a star or compact object moving through the ISM, or (4) an ionized trail left by photoionization (``Fossil \stromgren Trail'') from a star or compact object. We favor this last hypothesis, and derive some of the basic properties for an ionized trail. Regardless of whether this latter hypothesis applies to this specific filament, the basic properties of such a trail, its length, width, and brightness, are interesting, predictable, and should be observable behind some white dwarfs. We suggest future tests for ascertaining the origin of this filament, and discuss how this structure might be useful to constrain the thermal and velocity structure of the nearby interstellar medium.