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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...

Creating Ultra-Diffuse Galaxies

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Ultra-diffuse galaxies (UDGs) have very low luminosities, comparatively few stars, and little star-formation activity as compared with normal galaxies of similar sizes. Commonly found in ...

National Academies Releases ASTRO2020

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On Thursday, November 4, the National Academy of Sciences released the 2020 Decadal Survey, Pathways to Discovery in Astronomy and Astrophysics for the 2020s. The report identifies the mo...

Building Planets from Protoplanetary Disks

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Planets and their stars form from the same reservoir of nebular material and their chemical compositions should therefore be correlated but the observed compositions of planets do not mat...
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