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First Results from the Dark Energy Survey

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The Dark Energy Survey (DES) program uses the patterns of cosmic structure as seen in the spatial distribution of hundreds of millions of galaxies to reveal the nature of "dark energy," t...

The Interiors of Stars

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The interiors of stars are largely mysterious regions because they are so difficult to observe. Our lack of understanding about the physical processes there, like rotation and the mixing ...

Nick Rigby

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This is the body of my workspace.

The Center for Astrophysics Hosts a "Street" at the AAS

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For the first time, the Center for Astrophysics | Harvard & Smithsonian will host a "Street" at a conference. The 235th meeting of the American Astronomical Society being held this we...

Early Galaxies

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Galaxies that are very luminous in the infrared are generally active in making new stars whose ultraviolet radiation heats the dust. The energy, re-radiated by the dust at infrared wavele...

Blazar Variability

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Active galactic nuclei (AGN) are supermassive black holes at the centers of galaxies that are accreting material. These AGN emit jets of charged particles that move at speeds close to tha...

Galaxy Gathering Brings Warmth

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Cambridge, MA - As the holiday season approaches, people in the northern hemisphere will gather indoors to stay warm. In keeping with the season, astronomers have studied two groups of g...

Simulating Galactic Outflows

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Astronomers have known for decades that massive outflows of gas are being ejected from galaxies. These fast-moving, bipolar streams act to slow down the rate of star formation and inhibit...

Probing the Solar Wind Up Close

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The sun glows with a surface temperature of about 5500 degrees Celsius but its hot outer layer, the corona, has a temperature of over a million degrees. The corona ejects a wind of charge...
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