Interstellar Medium, Molecular Clouds, Star Formation & Evolution, Supernovae & Their Remnants, Long Gamma-ray Bursts, Cosmic Rays
Image credit: ALMA / ESO / NAOJ / NRAO / Alexandra Angelich, NRAO / AUI / NSF.
Stars are the fundamental building blocks and probes of the Universe. They are formed in stellar nurseries enshrouded by dust and gas, and end their lives in violent explosions, creating some of the most captivating events one can witness. Faculty in CIERA study, model, and observe many stages of a star’s life from birth to death, the planets formed around them, how they impact their environments, as well as the compact remnants they leave behind.
Research at CIERA
Evolving to the end states of stellar evolution, Professor Fong’s team uses radio and optical observations to study and model relativistic explosions called gamma-ray bursts and their host galaxy environments, probing star formation from the local neighborhood to the high-redshift Universe.
Professor Tchekhovskoy uses state-of-the-art simulations to study the formation of relativistic jets in core-collapse gamma ray bursts.
Professor Miller’s group uses ground- and space-based telescopes to study the endpoints of the stellar life cycle as punctuated by supernovae. The group uses data science methods, such as machine learning, to support the discovery and classification of these explosions prior to studying their properties in greater detail.
Professor Figueroa-Feliciano’s group studies the X-ray signatures of supernova remnants through the NASA Micro-X Sounding Rocket, a Northwestern-led rocket payload which takes high-energy-resolution spectra of remnants in suborbital flights.
Professor Kilpatrick uses optical, infrared, and X-ray imaging of nearby galaxies to understand the stellar channels that lead to their cataclysmic collapse and explosion as supernovae, focusing on deep, high-resolution imaging and spectroscopy that can be used to study their local environments, nucleosynthetic content, and progenitor stars.
News
Gallery
Brightest gamma-ray burst of all time came from the collapse of a massive star
Brightest gamma-ray burst of all time came from the collapse of a massive star
In October 2022, an international team of researchers, including Northwestern University astrophysicists, observed the brightest gamma-ray burst (GRB) ever recorded, GRB 221009A. In a paper published in April 2024, a team led by CIERA Postdoctoral Fellow Peter Blanchard has confirmed that the phenomenon responsible for the historic burst — dubbed the B.O.A.T. (“brightest of all time”)
Aaron M. Geller / Northwestern / CIERA / IT Research Computing and Data Services
- Science
Bursts of star formation explain mysterious brightness at cosmic dawn
Bursts of star formation explain mysterious brightness at cosmic dawn
Artist conception of early starbursting galaxies. Stars and galaxies are shown in the bright white points of light, while the more diffuse dark matter and gas are shown in purples and reds. When scientists viewed the James Webb Space Telescope’s (JWST) first images of the universe’s earliest galaxies, they were shocked. The young galaxies appeared
Aaron M. Geller, Northwestern, CIERA + IT-RCDS
- Science
Unprecedented gamma-ray burst explained by long-lived jet
Unprecedented gamma-ray burst explained by long-lived jet
Last year, Northwestern University researchers uncovered new observational evidence that long gamma-ray bursts (GRBs) can result from the merger of a neutron star with another compact object (either another neutron star or black hole) — a finding that was previously believed to be impossible. Now, another Northwestern team offers a potential explanation for what generated
Ore Gottlieb/Danat Issa/Alexander Tchekhovskoy/CIERA/Northwestern
- Science
‘Jupiter’ passed through massive stars
‘Jupiter’ passed through massive stars
A Northwestern University-led team of researchers, including postdoctoral fellow Evan Anders, developed the first 3D simulations of energy rippling from a massive star’s core to its outer surface. Using these new models, the researchers determined, for the first time, how much stars should innately twinkle. Depending on how large or bright a massive star is,
Northwestern University
‘Twinkle, Twinkle, Little Star’ passed through massive stars
‘Twinkle, Twinkle, Little Star’ passed through massive stars
A Northwestern University-led team of researchers, including postdoctoral fellow Evan Anders, developed the first 3D simulations of energy rippling from a massive star’s core to its outer surface. Using these new models, the researchers determined, for the first time, how much stars should innately twinkle. Depending on how large or bright a massive star is,
Northwestern University
Listen to a star ‘twinkle’
Listen to a star ‘twinkle’
A Northwestern University-led team of researchers developed the first 3D simulations of energy rippling from a massive star’s core to its outer surface. Using these new models, the researchers determined, for the first time, how much stars should innately twinkle. The team converted these rippling waves of gas into sound waves, enabling listeners to hear
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Core Faculty
Kari Frank
Director of Operations of CIERA, Research Assistant Professor
External Faculty
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