Unusual stellar nurseries near our galaxy’s center puzzle scientists

These images are made from data from the Stratospheric Observatory for Infrared Astronomy (SOFIA), the Spitzer Space Telescope, and the Herschel Space Observatory. Image credit: J. De Buizer (SETI) / SOFIA / Spitzer / Herschel

New research led by Dr. James De Buizer at the SETI Institute and Dr. Wanggi Lim at IPAC at Caltech revealed surprising results about the rate at which high-mass stars form in the galactic center of the Milky Way. The researchers based their study primarily on observations from NASA’s now-retired SOFIA airborne observatory, and using data from the U.S. National Science Foundation Very Large Array archive, and focuses on three star-forming regions—Sgr B1, Sgr B2, and Sgr C—located at the heart of the galaxy.

This science was presented at the 246th American Astronomical Society Conference in Anchorage, Alaska on Monday, June 9, 2025, 2:15 PM AK. You can read the full release from SETI.

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This news article was originally published on the NRAO website on June 13, 2025.