Supermassive, Intermediate & Stellar Mass Black Holes, White Dwarfs, Neutron Stars, Pulsars, Tidal Disruption Events
Image Credit: Aaron Geller/CIERA
Supermassive black holes at the centers of galaxies, elusive intermediate mass black holes, and dead stars in the form of black holes, neutron stars, or white dwarfs, are the densest objects in the Universe. They are central players in much of modern astrophysics, but we have only been aware of and studying these objects for less than a century. Our observational record is less than five decades long. As such, there are still many unanswered questions about how these systems form and evolve over cosmic time. CIERA is home to a broad group of researchers in theory, simulation, and observation that study these exotic objects.
Research at CIERA
Few things in the Universe are as dramatic as the death of a star. Transient events like supernovae, gamma ray bursts, and tidal disruptions of stars encountering massive black holes, are all astoundingly bright and carry information about the star that died, how it tore itself apart, and the fragments that remain.
Professor Fong observes short gamma ray bursts to learn about the neutron star and black hole mergers that give rise to these intense explosions.
Professor Miller observes Type Ia supernovae to understand the conditions and environments under which white dwarf stars explode.
Opportunities
Deadline: 11:59pm, March 20, 2023
REACH (Research Experiences in Astronomy at CIERA for High School Students) is a highly interactive, 3-week program (with an optional 3-week extension) that provides high school students experience with astronomy research in an atmosphere of team-style learning, hands-on training, and mentorship from professional scientists. Students enrolled in the program engage in astronomy research projects with CIERA astronomers.
News




Gallery

CIERA Interdisciplinary Colloquium: “Extremely Cool Detectors On a Fireball: Launching the Micro-X Sounding Rocket”
CIERA Interdisciplinary Colloquium: “Extremely Cool Detectors On a Fireball: Launching the Micro-X Sounding Rocket”
Professor Enectali Figueroa-Feliciano presents an Interdisciplinary Colloquium on December 1, 2022, organized by Northwestern University’s Center for Interdisciplinary Exploration and Research in Astrophysics. Read the full CIERA News story here.

Star Collapses into NEW Black Hole
Star Collapses into NEW Black Hole
Affectionately referred to as the B.O.A.T. (“brightest of all time”), the powerful explosion occurred approximately 2.4 billion light-years away from Earth, in the direction of the constellation Sagitta. Astrophysicists, including Jillian Rastinejad, first detected the GRB, which was a few hundred seconds in duration, in gamma-ray light on Oct. 9. Read the full Northwestern News
National Science Foundation

Short gamma-ray bursts traced farther into distant universe

Short gamma-ray bursts traced farther into distant universe
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.
W.M. Keck Observatory/Adam Makarenko

X-shaped Radio Galaxy Morphology: 3-dimensional movie of density
X-shaped Radio Galaxy Morphology: 3-dimensional movie of density
When astronomers use radio telescopes to gaze into the night sky, they typically see elliptical-shaped galaxies, with twin jets blasting from either side of their central supermassive black hole. But every once in a while — less than 10% of the time — astronomers might spot something special and rare: An X-shaped radio galaxy, with
Aretaios Lalakos

X-shaped radio galaxies might form more simply than expected

X-shaped radio galaxies might form more simply than expected
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
Aretaios Lalakos

Northwestern’s ‘Micro-X’ rocket to image supernova remnant (b roll)
Northwestern’s ‘Micro-X’ rocket to image supernova remnant (b roll)
On Aug. 21, 2022, a NASA-funded Northwestern University team of astrophysicists 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
Northwestern University
People
Core Faculty






Vicky Kalogera
Daniel I. Linzer Distinguished University Professor, Director of CIERA

Shane Larson
Research Professor, Associate Director of CIERA






Associate Faculty

Postdocs









Research Staff


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