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| The Southern Ring Nebula, or NGC 3132, was one of the first objects observed by the James Webb Space Telescope. Image Credit: NASA/ESA/CSA/STScI |
Planetary nebulae have been studied for centuries, but astronomers are getting new looks and a better understanding of the structures and compositions of these gaseous remnants of dying stars thanks to the ability to study objects at multiple wavelengths and dimensions.
The Southern Ring Nebula, or NGC 3132, is one such object. Rochester Institute of Technology Chester F. Carlson Center for Imaging Science and School of Physics and Astronomy Professor Joel Kastner and his team used Submillimeter Array (SMA) mapping to take a closer look at the nebula, which was one of the first cosmic objects observed by the James Webb Space Telescope soon after its deployment in 2022. The researchers found that most of the molecular gas in the nebula actually lies in an enormous, expanding ring, and further, that the nebula has a second, nearly perpendicular, expanding ring. The research findings were recently published in The Astrophysical Journal. Kastner is the founding director of RIT’s Laboratory for Multiwavelength Astrophysics.
Inspired by the JWST infrared images, which dramatically reveal how hydrogen gas in molecular form threads through the Southern Ring, Kastner and the team used SMA radio-wavelength mapping to measure both the distribution on the sky and the precise velocities of carbon monoxide gas in the nebula. The measurements establish which regions of the Southern Ring Nebula are moving toward and away from us, revealing the two rings. The team’s new SMA results support previous findings that the nebula’s present form is the result of interactions between the dying star and one or possibly two companion stars.


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