The discovery of the largest gas filament in our Galaxy, or a new spiral arm?
Chong Li, Keping Qiu, Bo Hu, and Yue Cao

TL;DR
Using FAST, we discovered the largest known gas filament in our Galaxy, named Cattail, which challenges existing models of Galactic structure and may represent a new spiral arm or an extension of known features.
Contribution
We identified and characterized the largest giant HI filament in the Galaxy, providing new insights into Galactic structure and the potential existence of a new spiral arm.
Findings
Cattail is 1.1 kpc long, possibly extending to 5 kpc.
It has a mass of 6.5 × 10^4 solar masses.
Cattail's location suggests it may be part of a new Galactic arm or extension.
Abstract
Using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), we detect a giant HI filamentary structure in the sky region of 3077 3110 and 409 434. The structure has a velocity range of 170 km s to 130 km s, and a mean velocity of 150 km s, putting it to a Galactocentric distance of 22 kpc. The HI structure has a length of 1.1 kpc, which appears to be so far the furthest and largest giant filament in the Galaxy and we name it Cattail. Its mass is calculated to be 6.5 10 M and the linear mass density is 60 M pc. Its width is 207 pc, corresponding to an aspect ratio of 5:1. Cattail possesses a small velocity gradient (0.02 km s pc) along its major axis. Together with the HI4PI data, we find that Cattail…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
