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Measuring Galaxy Evolution with Globular Clusters

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Globular clusters are gravitationally bound ensembles of stars, as many as a million stars in some cases, grouped in roughly spherical clusters with diameters as small as only tens of lig...

Cosmic Bumps on Cosmic Ripples

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In 1969, the astrophysicists Rashid Sunyaev and Yakov Zel'dovich realized that the then recently discovered cosmic microwave background radiation (CMBR) would be distorted by hot cosmic g...

BICEP: From the South Pole to the beginning of time

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It's a little known fact that three-quarters of a mile from the South Pole lie some of Earth's most powerful telescopes. Operated all year round, they are engaged in one of the great scie...

Nanodust Particles in the Interplanetary Medium

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Dust particles smaller than about a wavelength of light are abundant in our solar system, created by collisions between asteroids and from the evaporation of comets. As they scatter sunli...

Where Do Stars Form in Merging Galaxies?

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Collisions between galaxies, and even less dramatic gravitational encounters between them, are recognized as triggering star formation. Observations of luminous galaxies, powered by star...

Chandra Finds Intriguing Member of Black Hole Family Tree

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A newly discovered cosmic object may help provide answers to some long-standing questions about how black holes evolve and influence their surroundings, according to a new study using NAS...

Quadruplets in a Stellar Womb

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More than half of all stars are in multiple systems: binary stars, or even triplets or quadruplets, that orbit one another. No one is quite sure how or why they form, but the effects can...
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