arXiv · astro-ph/0205032
Expanding shells of shocked neutral hydrogen around compact HII regions
Abstract
By comparing radial velocities of radio bright compact HII regions with their HI absorption profiles, we discovered expanding shells of neutral hydrogen around them. These shells are revealed by absorption of the radio continuum emission from the HII regions at velocities indicating greater distances than the observed radial velocity. We believe that these shells are shock zones at the outer edge of the expanding ionized region. Additionally we found evidence for a velocity inversion inside the Perseus arm caused by a spiral shock, which results in a deep absorption line in the spectra of compact HII regions behind it.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Roland Kothes, Charles R. Kerton. 2002-05-02. Expanding shells of shocked neutral hydrogen around compact HII regions. https://doi.org/10.1051/0004-6361%3A20020671
Cite the original work for its findings. Save a collection to share your selection of sources.