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A Galaxy Cluster with Two Pairs of X-Ray Cavities

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Supermassive black holes (SMBH) at the centers of galaxies sometimes accrete material onto a surrounding torus of gas and dust. When this happens, the material is heated to thousands of d...

Exoplanets in Debris Disks

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Debris disks around main-sequence stars are tenuous belts of dust thought to be produced when asteroids or other planetesimals collide and fragment. They are common: more than about a qua...

The Role of Turbulence in Making Massive Stars

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Molecular clouds in the Milky Way are generally very inefficient in forming stars; only about 1% of the available material ends up in a star. Astronomers think one reason is that star-for...

The Host Galaxy of a Fast Radio Burst

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Fast radio bursts (FRBs) are bright pulses of emission at radio wavelengths (seen mostly at wavelengths of tens of centimeters) whose physical mechanism(s) are mysterious. The bursts last...

Active Galactic Nuclei and Galaxy Cluster Cooling

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Galaxy clusters are the largest and most recently formed structures in the universe. The closest large cluster of galaxies to us is the Virgo Cluster with about 2000 members. (The Milky W...

Giant Magellan Telescope Ranked a National Priority

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Pasadena, CA -- The 2020 Decadal Survey for Astronomy and Astrophysics has recommended federal support for the final construction stages of the Giant Magellan Telescope (GMT) as part of t...
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