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The kilonova and gamma-ray burst is on the right. The blue color represents material squeezed along the poles, while the red colors indicate material ejected by the two inspiralling neutron stars that is now swirling around the merged object. A disk of ejecta emitted after the merger, hidden behind the red and blue ejecta, is shown in

Artist’s impression of STAR-X after its proposed launch in 2028. The aperature of the X-ray telescope is the large circular shape toward the left. The ultraviolet telescope is the outrigger tube attached to the facility’s underside.

A Northwestern University-led team of astronomers has developed the most extensive inventory to date of the galaxies where short gamma-ray bursts (SGRBs) originate. Using several highly sensitive instruments and sophisticated galaxy modeling, the researchers, including Anya Nugent, pinpointed the galactic homes of 84 SGRBs and probed the characteristics of 69 of the identified host galaxies.

“This GRB is an extraordinarily rare event,” said Rastinejad, a Northwestern Ph.D. student. “It was so bright that it triggered the Swift gamma-ray telescopes twice and fully saturated the detectors — something I haven’t seen in my time observing GRBs.” “As long as we have been able to detect GRBs, there is no question that

On Aug. 21, a NASA-funded team that includes Northwestern faculty and students launched the “Micro-X” rocket from White Sands Missile Range in southern New Mexico. The rocket spent 15 minutes in space — just enough time to snap a quick image of supernova remnant Cassiopeia A, a star in the Cassiopeia constellation that exploded approximately

For the first time, the James Webb Space Telescope has been used to directly image an exoplanet — that’s a planet outside of our solar system. Although it’s not the first time an exoplanet has been directly imaged, it is the first time the Webb Telescope’s powerful gaze has been turned to the task. And

This image shows the exoplanet HIP 65426 b in different bands of infrared light, as seen from the James Webb Space Telescope: purple shows the NIRCam instrument’s view at 3.00 micrometers, blue shows the NIRCam instrument’s view at 4.44 micrometers, yellow shows the MIRI instrument’s view at 11.4 micrometers, and red shows the MIRI instrument’s

A team at Northwestern University spent a decade working on a rocket. The goal was to send it to space to take an image of the supernova remnant Cassiopeia A, a star in the constellation that exploded. On August 21, 2022, the team launched their rocket. “People just went wild,” said Tali Figeroa-Feliciano, project lead.

A still image taken from the 3D simulation of the natural development of an X-shaped jet. The gas (bright red) falls into the black hole, which launches a pair of relativistic jets (light blue). The jets propagate vertically and shock the ambient gas (dark red). The older cavities (dark blue) buoyantly rise at an angle

On Aug. 21, the NASA-funded team launched its “Micro-X” rocket from White Sands Missile Range in southern New Mexico. The rocket spent 15 minutes in space — just enough time to snap a quick image of supernova remnant Cassiopeia A, a star in the Cassiopeia constellation that exploded approximately 11,000 light-years away from Earth. Then,

In a new study, the team of astrophysicists who launched STARFORGE discovered that star formation is a self-regulatory process. In other words, stars themselves set their own masses. This helps explain why stars formed in disparate environments still have similar masses. The new finding may enable researchers to better understand star formation within our own Milky